The galaxy appears as a centrally concentrated, elliptical structure. It exhibits a smooth, featureless morphology with no discernible spiral arms or bar. The light profile suggests a gradual decline in brightness from the core outwards. The object shows a slight elongation, more so than it is rounded, but is not overtly cigar-shaped. There are no indications of any major mergers or tidal disturbances in its immediate vicinity, although there may be minor disturbances. The galaxy has a yellow-orange hue, which implies a population of older stars with low star formation activity. The small apparent size and red color suggest this galaxy is at a significant distance.
