The galaxy presents as a relatively smooth, elliptical-like structure with a pronounced central bulge. There is a slight elongation evident, giving it a somewhat cigar-shaped appearance. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The color profile suggests an older stellar population, as it exhibits a yellowish-red hue, with a very small amount of blue visible on the edges, suggesting that it is very weakly forming stars. The overall structure appears largely undisturbed, lacking any obvious signs of a major ongoing or recent merger event.
