The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. The core appears bright and nearly spherical, gradually decreasing in intensity towards the outer edges. The galaxy's color profile displays a yellowish hue, indicative of an older stellar population with fewer young, blue stars. There is no discernible spiral structure or significant dust lane features. However, the smooth light profile is slightly disturbed suggesting a possible tidal interaction or past merger event. Faint color variations are noticeable in the outskirts, which might imply ongoing star formation at a low rate.
