The galaxy appears as a centrally concentrated object, approximately elliptical in shape, although precise determination is hindered by image resolution. A dominant, smoothly distributed component is observed. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. There is a subtle color gradient, shifting towards a redder tone in the outer regions compared to the core. No distinct spiral arm structures, dust lanes, or prominent star-forming regions are discernible. There are no significant tidal features, such as streams or shells, indicating a relatively quiescent recent merger history. The overall morphology suggests an evolved system with minimal ongoing star formation. The galaxy's size seems relatively compact.
