The galaxy presents a largely elliptical morphology. Its core exhibits high luminosity, suggesting a dense concentration of stars. The overall color profile indicates a population of older stars, with a redder hue dominating the galaxy's outer regions. The galaxy appears relatively smooth, showing little evidence of significant spiral arm structure or prominent dust lanes. Faint blue regions are visible in the disk, suggesting recent star formation. There is a slight flattening visible in the galaxy's overall shape, deviating from a perfectly circular profile. No obvious signs of a major ongoing merger are apparent, although minor disturbances cannot be ruled out based on the image alone. The lack of strong tidal features supports the conclusion that the galaxy is relatively isolated and undisturbed.