The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. Its light distribution is not perfectly circular, showing a slight elongation. The core region exhibits a bright, yellowish-orange hue, likely indicating an older stellar population. The outer regions display a gradual fading and color shift to a slightly bluer tint, suggesting the presence of some younger stars, although the overall color profile implies a predominantly evolved population. There is no strong evidence of spiral arms or significant dust lanes. The galaxy does not appear to be undergoing a major merging event, though the possibility of minor tidal disturbances can’t be ruled out based on this image alone. The overall form suggests a galaxy in a relatively late stage of its evolution.
