The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears bright, with a color gradient transitioning from a yellowish core to a slightly bluer outer region. No distinct spiral arm structures or prominent dust lanes are apparent. The overall roundness suggests a classification leaning towards an E0-E3 elliptical. There appears to be little to no signs of ongoing mergers or significant tidal disturbances within the visible structure. The galaxy's light profile suggests a relatively old stellar population, and it shows signs of modest star formation.
