The galaxy appears as a slightly elongated, lenticular-like structure. It has a smooth, diffuse appearance with a concentration of light towards the center, suggesting a prominent bulge. There is a subtle disk component, although the overall morphology is dominated by the bulge. The galaxy exhibits a yellowish-white color, indicative of an older stellar population and minimal ongoing star formation. There is no obvious sign of a spiral arm structure, although this may be due to its viewing angle. There is a hint of minor disturbance in the galactic halo, suggestive of either an on going or past merger event with a smaller galaxy.
