The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge with a yellowish-white hue, indicating an older stellar population. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy has a generally rounded morphology, showing minimal signs of tidal disturbances or ongoing mergers. The outer regions of the galaxy appear fainter and redder, suggesting a decreasing density of stars and a shift towards older, redder stars in the outskirts. Overall, the galaxy seems to be a fairly evolved system, likely with a high mass and a relatively low rate of star formation.
