The galaxy presents as a lenticular or early-type spiral, possibly viewed at a moderate inclination. A prominent central bulge dominates the structure, appearing relatively smooth and concentrated, indicating an older stellar population. The disk component appears faint and somewhat diffuse with subtle hints of spiral arms and possibly a dust lane near the galactic plane. The galaxy exhibits a general color profile, with the central bulge trending towards yellower hues, suggestive of older, redder stars, while the disk shows bluer tones, possibly indicating regions of recent star formation. There is no obvious evidence of a recent major merger. There appear to be minor disturbances such as a slight asymmetry in the distribution of light in the outer disk. The overall morphology suggests a system that is in a relatively quiescent state.
