The galaxy presents an elongated, disk-like structure, suggestive of a spiral or lenticular galaxy viewed at a high inclination, approaching edge-on. The central region exhibits a bright, concentrated bulge that transitions smoothly into the surrounding disk.

The disk displays a color gradient, with the central bulge appearing more yellow-red, indicative of an older stellar population. Towards the edges of the disk, the color shifts to a bluer hue, potentially indicating the presence of younger, hotter stars and ongoing star formation regions. There is a slight lopsidedness to the visible disk, which may be intrinsic, or due to tidal interactions.

The absence of clearly defined spiral arms suggests a relatively smooth stellar distribution within the disk, potentially consistent with a more evolved spiral or lenticular type. Faint dust lanes appear present near the central bulge, possibly obscuring some of the light from background stars. No major disturbances are visible, suggesting a relatively isolated system that is not undergoing a major merger.

The overall morphology indicates a galaxy with a moderate stellar mass and star formation rate.
