The galaxy presents as a relatively smooth, centrally concentrated elliptical. It exhibits a generally round morphology with a bright, compact core. The color profile suggests a dominant population of older stars, indicated by the yellowish-white hue towards the central region. There is a subtle blue tinge in the outer regions of the halo, hinting at a small amount of ongoing star formation. No prominent spiral arms or significant dust lanes are discernible. There is no significant tidal distortion or any indication of a major ongoing merger. There may be a very small amount of disturbance.
