The galaxy presents as a relatively compact elliptical or lenticular type. It exhibits a smooth, concentrated luminosity profile, brightest towards the center, with a rapid decrease in intensity outwards. The overall shape is elongated, showing a slight elliptical structure. Color gradients are visible, with the central region displaying a yellower hue, suggestive of an older stellar population dominated by red giant stars. The outer regions show some bluer tones, hinting at the presence of younger, hotter stars, and a faint disk component that might have some star formation occurring. There is no strong evidence of spiral arms or significant dust lanes. The galaxy does not display any signs of major mergers or significant tidal disturbances.
