The galaxy appears to be elliptical in shape, presenting as a somewhat elongated spheroid. The central region exhibits a concentration of luminosity, suggesting a prominent galactic nucleus. The galaxy displays a generally smooth texture with no obvious spiral arm structures or distinct dust lanes. The color profile is predominantly yellow-white, which likely indicates an older stellar population. The outer regions exhibit a gradual decline in luminosity, merging into the background sky. There is a subtle indication of minor structural asymmetry in the form of a slight distortion. No obvious signs of ongoing major mergers are apparent; however, the slight distortion could indicate recent or ongoing minor interaction.
