The galaxy appears as a centrally concentrated, relatively smooth structure. Its shape is somewhat elliptical, with the light distribution gradually decreasing from the core outwards. There are no visually distinct spiral arms or prominent features indicative of active star formation regions. The overall color is a yellow-white hue, suggesting a population dominated by older stars and a lack of substantial dust obscuration. Given its morphological properties, it seems likely to be an early-type galaxy, potentially an elliptical or lenticular galaxy viewed at a distance where finer details are not easily resolved. There is no obvious ongoing merger activity or significant tidal disturbances.
