The galaxy appears as a generally smooth, elliptical structure. Its color profile suggests a primarily older stellar population, with a yellowish-red hue concentrated towards the central region, indicative of evolved stars. There's little evidence of significant dust lanes or spiral arm structures. The light distribution is highly concentrated towards the center, with a gradual decrease in intensity extending outward. It exhibits a relatively round morphology, with no obvious signs of ongoing major mergers or tidal disturbances. Faint, diffuse light extends beyond the core, suggesting a halo of stars.
