The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical, exhibiting a gradual decrease in brightness from the core outwards. There is no discernible spiral arm structure or prominent dust lanes visible. The central region is bright, suggesting a high concentration of stars or potentially an active galactic nucleus, though this cannot be confirmed from the image alone. The galaxy appears to be in a relatively isolated state, showing no obvious signs of major interaction or merging with other galaxies, though minor disturbances cannot be entirely ruled out. The color profile appears relatively uniform across the galaxy. The image suggests a galaxy with an older stellar population and low star formation rate.
