The galaxy presents a smooth, elliptical morphology. It appears to be a relatively compact object, exhibiting a generally round shape with minimal discernible features beyond a central concentration of light. The color index suggests a population of older stars, resulting in a reddish-yellow hue. There is little evidence of active star formation regions or spiral arm structures. No distinct tidal tails or other indicators of recent or ongoing major mergers are apparent, although there is some slight asymmetry which may be due to a minor disturbance. The galaxy is likely a massive system, as indicated by its high luminosity.