The galaxy presents as an elliptical morphology, appearing largely smooth and rounded. The color profile indicates a redder hue, suggesting an older stellar population. There is no strong evidence of spiral arm structure or a prominent disk. The overall light distribution is centrally concentrated, without significant irregularities or tidal features, indicating a lack of major mergers or interactions. A slight asymmetry may hint at a minor disturbance or interaction, but this is not definitive. The galaxy appears relatively isolated within its immediate surroundings.
