The galaxy presents as an elliptical morphology, characterized by a smooth, largely featureless light distribution. The core exhibits a reddish hue, suggestive of an older stellar population. Surrounding the core is a more diffuse, greenish halo, potentially indicating ongoing or recent star formation activity in the outer regions. There is a slight elongation in shape, deviating marginally from a perfect sphere, and the overall structure appears undisturbed, showing no signs of significant tidal interactions or major mergers. The galaxy is relatively compact.
