The galaxy presents a primarily smooth, elliptical morphology. The central bulge exhibits high luminosity, appearing as a bright, concentrated core. The outer regions of the galaxy gradually fade, forming a diffuse halo. There is very little discernible disk structure or prominent spiral arms. The overall color profile suggests a population of older stars, with subtle variations in color across the galaxy's surface. No significant dust lanes or active star-forming regions are immediately apparent. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or major mergers. A slight asymmetry or minor disturbance may be present but is very subtle. The estimated physical size is moderate. The light emitted indicates a relatively low star formation rate, suggesting an older stellar population. The total mass is substantial, indicative of a mature galaxy.
