The galaxy presents a generally smooth, elliptical morphology. It appears to be relatively undisturbed, showing no strong evidence of ongoing mergers or tidal interactions. The light distribution is centrally concentrated, with a gradual decline in brightness towards the outer regions. Color gradients are subtle, with a slightly bluer core transitioning to a redder halo. There is no discernible dust lane, and any star-forming regions are not prominently visible. The overall structure suggests a galaxy dominated by an older stellar population and a lack of significant recent star formation. The galaxy's round shape further supports the elliptical classification.
