The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It exhibits a primarily rounded morphology, lacking any clear spiral arm structures or a distinct disk. There is no evidence of strong tidal features or ongoing major mergers, although some slight asymmetry may hint at a minor interaction or past disturbance. The galaxy displays a gradual decline in luminosity from its core outwards. The color profile suggests a population dominated by older stars, with a somewhat redder hue overall. While largely smooth, a faint, diffuse outer halo is visible, extending beyond the main body of the galaxy.
