The galaxy presents as a relatively smooth, centrally concentrated object, appearing mostly featureless at this resolution. The light distribution suggests a roughly elliptical morphology, with a high degree of central symmetry. There is little evidence of spiral arms or a prominent disk structure. The color profile indicates a population dominated by older stars, with a yellowish to slightly reddish hue, potentially indicating a lack of significant ongoing star formation. There is a slight elongation along one axis. This galaxy appears to be a relatively undisturbed system, with no obvious signs of recent major mergers or tidal interactions. However, there are subtle hints of minor disturbances in its outer regions, which might be indicative of past interactions.
