The galaxy presents a generally smooth, elliptical morphology. It displays a centrally concentrated luminosity profile, appearing brightest at its core and gradually fading outwards. The overall shape is close to round, with a slight deviation towards an intermediate elliptical form. There is no obvious evidence of a prominent disk structure or spiral arms. The galaxy appears to be isolated, with no strong indications of ongoing major mergers or significant tidal disturbances, although there may be minor irregularities within the galaxy. The color index suggests a population of older stars, contributing to the reddish-yellow hue. This galaxy appears to be a relatively massive and passive system, with a low rate of star formation activity.