The galaxy appears to be a lenticular or edge-on spiral galaxy. Its morphology is predominantly smooth, with a central bulge that appears yellowish-white in color, indicative of an older stellar population. The disk of the galaxy is elongated, with a cigar-like shape. A blueish hue along the edges of the disk suggest the presence of younger, hotter stars and possibly ongoing star formation, though this activity is limited. There are no major disturbances or signs of merging present. The galaxy does not show a strong spiral structure when viewed from our angle. The light distribution indicates a relatively high mass. Overall, the galaxy presents as an evolved system transitioning away from active star formation.
