The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge exhibits a concentrated luminosity, appearing yellowish-white, indicative of an older stellar population. Fainter, bluer light surrounds the central bulge, possibly hinting at some ongoing, albeit low-level, star formation in the outer regions. There is no evidence of a strong disk component or spiral arm structure. The galaxy appears to be fairly undisturbed, without major signs of tidal interactions or recent mergers. A slight elongation is observed, with the major axis extending horizontally across the image.
