The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution. The core region exhibits a brighter, more concentrated luminosity. Faint extensions are barely visible with the resolution provided. There appears to be a slight change in color with galactocentric radius, with a redder tone near the core. The overall form does not show evidence of spiral arms or significant irregular features; rather, a flattened spheroid shape is observed. No pronounced dust lanes or recent star formation are distinctly visible. The galaxy's classification is likely an early-type galaxy. There is some evidence of possible minor tidal disturbances, potentially from a nearby companion, but this is not clear and requires more investigation. The object seems to be relatively isolated.
