The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears relatively uniform, fading gradually from the core outwards. There are no prominent spiral arms or significant dust lanes visible. The color profile suggests a population of older stars, as indicated by the reddish hue. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or recent merger events in this image, although very faint disturbances may be present. Based on its morphology and color, this galaxy is likely an early-type galaxy with suppressed star formation.
