The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth, diffuse light distribution. There is no obvious spiral arm structure. The galaxy presents a centrally concentrated bulge, with the light intensity diminishing gradually toward the outer regions. The core exhibits a yellow-orange hue, suggesting an older stellar population. Moving outward from the core, the color shifts slightly towards a bluer tint, possibly indicating younger stars and ongoing star formation in the surrounding regions. There is a slight asymmetry to its overall shape, being somewhat elongated. No major interactions or tidal disturbances from nearby galaxies are apparent, but there might be a minor disturbance.
