The galaxy presents as a fairly smooth, elliptical structure, with a concentrated central bulge that gradually diffuses outwards into the surrounding halo. The light distribution appears relatively uniform, indicative of an older stellar population dominating the overall luminosity. The galaxy exhibits a slight elongation. There is an additional blue structure near the galaxy. Although I cannot distinguish the structure as being part of the galaxy, or if it is a foreground or background object. The lack of distinct spiral arms or prominent dust lanes further supports the classification as an early-type galaxy. Overall, the observed characteristics suggest a well-evolved system with limited ongoing star formation activity.
