The galaxy appears to be relatively compact, with an overall elliptical morphology. The light distribution seems concentrated towards the core, with a noticeable color gradient suggesting variations in stellar populations or dust content. There is some subtle irregularity to the outer edges of the galaxy's light profile, which could be evidence of tidal interactions or past mergers. The inner region exhibits a bright core, possibly indicating the presence of an active galactic nucleus. The lack of clearly defined spiral arms, or a prominent disk structure indicates the galaxy may be an elliptical type.
