The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The light distribution suggests a higher density of stars towards the center, gradually decreasing outward. The color profile indicates a dominant population of older stars, contributing to the yellowish hue. There is some subtle indication of a disk, but it is not prominent. No distinct spiral arms or significant dust lanes are visible. The galaxy appears undisturbed with no signs of a major merger event. The shape appears somewhere in between round and cigar-shaped. There are no features indicating active star formation regions.
