The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge that appears to be its dominant feature. The light distribution suggests that it is an older galaxy, with a lack of spiral arm structure. The galaxy appears elongated, almost cigar-shaped, indicating a deviation from perfect circularity. There is no clear evidence of ongoing major merging activity, although a slight asymmetry in its outer regions could suggest a minor interaction or disturbance. The overall color is indicative of a population of older stars, with lower levels of ongoing star formation.
