The galaxy presents a predominantly smooth, elliptical morphology, with a slight elongation. Its color gradient suggests an older stellar population, potentially indicative of a relatively quiescent state of star formation. The central region exhibits a concentrated luminosity, fading smoothly towards the outer edges. There is a suggestion of a slight disturbance or feature located nearby but could also be an artifact. The overall structure appears relatively undisturbed, showing no significant signs of ongoing major mergers or tidal interactions.
