This galaxy presents as an elliptical or lenticular type. Its overall appearance is largely smooth and symmetrical with a concentrated central bulge. The light distribution suggests a centrally concentrated luminosity profile, fading gradually outwards. There is some evidence of a faint, diffuse disk. The galaxy's color is predominantly yellowish-orange, indicating a relatively old stellar population. No prominent dust lanes or spiral arm structures are visible. There is no indication of any ongoing major merging events or significant tidal disturbances.
