The galaxy presents as a fairly compact, elliptical-like structure. Its light profile appears relatively smooth and centrally concentrated, indicating a possible lack of significant star formation or prominent spiral arms. The galaxy's color is somewhat uniform, exhibiting a slight yellowish-white hue, which suggests an older stellar population and a relatively low rate of ongoing star formation. There is no obvious dust lane or tidal features, which could indicate that it has not been disturbed by any recent mergers.
