This galaxy presents as a moderately compact structure. The light profile appears centrally concentrated, exhibiting a smooth, diffuse morphology without prominent spiral arms or a distinct bar. A slight elongation is discernible, though the overall shape is generally elliptical. The galaxy appears to be undergoing some form of interaction, with a degree of asymmetry and possibly tidal features or disturbances visible in its outer regions. There may be minor disturbances, indicating recent or ongoing mergers with smaller galaxies. Color gradients are subtle, with a suggestion of bluer hues in the central region compared to the redder outer edges, indicative of younger stellar populations concentrated towards the core.
