The galaxy presents as a relatively compact object. It appears to exhibit a smooth overall morphology, with a centrally concentrated luminosity profile. There is a slight suggestion of asymmetry in its outer regions, but no readily discernible spiral arms or distinct disk features are apparent. The color distribution is mostly uniform across the galaxy's extent, hinting at a fairly homogeneous stellar population. There is no obvious evidence of tidal tails, bridges, or other structures indicative of a recent or ongoing major merger event. Overall, this appears to be a galaxy consistent with an elliptical classification, with possible minor disturbances.
