The galaxy presents as a relatively smooth, elliptical structure. Its core region exhibits a concentrated luminosity, appearing more yellow-red in color. This could be attributed to an older stellar population dominating the central area. Moving outward from the core, the galaxy displays a more diffuse halo, tinged with hints of bluer hues. This suggests the presence of some younger, star-forming regions, although these seem less prominent compared to the overall stellar population. The galaxy's shape appears nearly round. There are no visually apparent signs of significant tidal disturbances or ongoing mergers, although the possibility of minor interactions cannot be ruled out. The overall morphology points towards a system that is relatively settled and evolved, with a low rate of current star formation.
