The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a more diffuse halo extending outwards. The color appears to be predominantly yellow/orange, suggesting a population of older stars and a relatively low rate of ongoing star formation. There may be some minor asymmetry, though the galaxy does not appear to be undergoing any major merger events. There are potentially some disturbances on the outer edges of the galaxy. Overall, the galaxy appears to be a somewhat evolved, massive system, likely dominated by an older stellar population.
