The galaxy appears to be a relatively smooth, elliptical type. Its overall shape is somewhat rounded, though not perfectly circular. A bright central bulge is evident, with the light intensity decreasing gradually towards the outer edges of the galaxy. There is little indication of spiral arm structure or significant dust lanes. The color profile suggests an older stellar population, with a yellow to reddish hue dominating the central regions. The outer regions appear slightly bluer, hinting at the presence of some younger stars, though star formation appears to be generally low overall. There is no obvious evidence of ongoing merging activity or major disturbances in its structure. The galaxy seems to be a fairly quiescent system.
