The galaxy exhibits a flattened, elliptical morphology, possibly an early-type spiral viewed at a high inclination. A prominent, bright central bulge dominates the overall structure. The bulge appears to be relatively smooth, lacking significant dust lanes or distinct features. Fainter, extended disk components are visible around the bulge; however, they are diffuse and poorly resolved in this image. There appears to be a blue-ish region offset from the galaxy's center that could indicate an area of star formation. The overall color index suggests a population of relatively old stars, but the offset could indicate an area of ongoing star formation. There is a slight indication of possible disturbances in the outer disk, hinting at a past or ongoing interaction, but the evidence is ambiguous. The galaxy's surface brightness decreases gradually from the bulge outwards, lacking the sharp edges often associated with late-type spiral galaxies. Overall, this galaxy displays characteristics of a disk galaxy with a large bulge, and the colors suggest a relatively old stellar population.
