The galaxy presents as a relatively smooth, elliptical-like structure. Its core is noticeably brighter, exhibiting a concentrated luminosity suggesting a substantial stellar density. The light distribution gradually diminishes from the central region outwards. The overall hue is indicative of an older stellar population. The galaxy appears to have a slight disk-like component with a more concentrated center. There is no evidence of significant spiral arm structure or ongoing major merger activity; instead, it appears relatively undisturbed. The shape is somewhat elongated, but predominantly rounded with no significant tidal tails or other signs of recent interaction. Based on the color gradients, the galaxy shows a relatively low rate of current star formation.
