The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that gradually fades into the outer regions. There is a slight elongation along one axis, deviating from a perfectly circular shape. A faint disk-like structure is potentially present, but the primary characteristic is a smooth, spheroidal distribution of light. The galaxy's color profile suggests a population of older stars, with a yellow-orange hue dominating the core. There may be some minor disturbances in the morphology but for the most part, it appears to be fairly stable, with no obvious major mergers or tidal features.
