The galaxy presents as an elliptical morphology with a smooth, centralized light distribution. The core region is relatively bright, exhibiting a yellowish hue, suggesting a population of older stars. Moving outwards, the light gradually diminishes and reddens slightly. The overall shape appears somewhat flattened. There is no distinct spiral arm structure or notable dust lane obscuration visible. The galaxy appears relatively isolated, with no immediately obvious signs of tidal interactions or recent merger events.
