The galaxy appears as a relatively small, luminous object with an overall smooth morphology. It exhibits a concentrated central region that gradually fades outwards, suggesting a lack of significant spiral arm structure or prominent features. The shape appears mostly circular. The color profile indicates a yellowish-white hue, possibly indicative of an older stellar population. There might be some minor indications of a slight irregularity in its form, suggesting a potential past interaction or disturbance. The galaxy is not displaying any significant signs of a major ongoing merger.
