The galaxy presents as a single, moderately concentrated object with a generally elliptical morphology. It exhibits a smooth, diffuse appearance, lacking any prominent spiral arms or a distinct bar structure. The light distribution suggests a relatively homogeneous stellar population, with a color gradient that appears somewhat redder towards the central region. There are no clear indications of ongoing major mergers or strong tidal features, although subtle disturbances cannot be ruled out given the resolution of the image. The galaxy appears relatively isolated within its immediate surroundings, showing no obvious signs of interaction with other nearby galaxies.
