The galaxy presents as a somewhat diffuse, elliptical-like structure with a noticeable central bulge. There appears to be a degree of disturbance in the morphology, possibly indicative of a minor merger event or tidal interaction. The color profile suggests a population of older stars, likely residing within the bulge, with bluer hues scattered throughout. The galaxy's overall shape is elongated, not perfectly spherical, appearing somewhat cigar-shaped. There is some evidence of disruption or asymmetry, possibly due to interactions, indicating recent or ongoing star formation. The light distribution is relatively smooth, with a higher concentration towards the center.
