The galaxy appears to be a relatively smooth, elliptical galaxy, possibly an early-type spiral viewed at an angle. It exhibits a concentrated, bright central bulge that gradually fades into a more diffuse halo. The galaxy's overall shape is somewhat elongated, displaying a moderate ellipticity but not appearing strongly barred or cigar-shaped. There is no apparent presence of defined spiral arms or prominent dust lanes. A slight asymmetry in the outer regions may suggest a past or ongoing minor interaction, but the overall morphology indicates it is not in the midst of a major merger. The color profile suggests an older stellar population, predominantly yellow-red in the central regions, possibly due to the light from older and redder stars.
