The galaxy presents as a relatively smooth, centrally concentrated system. Its morphology is largely elliptical, appearing significantly rounded. The luminosity profile suggests a concentrated core region which fades gradually into the outer regions. There is some indication of a possible disk-like structure, or at least some features beyond a perfectly smooth spheroid. No prominent spiral arms or bars are visible. There might be minor disturbances suggesting past interaction or possibly an ongoing merger event, but overall the system appears reasonably settled. Color gradients are subtle, with a generally yellowish hue, suggesting an older stellar population and/or significant dust extinction.
