The galaxy presents as a somewhat amorphous, diffuse structure, with a brighter central region. The overall shape appears elongated, with a suggestion of tidal features extending from the main body. The light distribution is uneven, hinting at possible disturbances. The color gradient suggests that the central region may be dominated by older stellar populations, whereas bluer tints extending outward hint at ongoing or recent star formation. There are indications of possible merging activity due to the irregular morphology and the tidal features. The galaxy is overall of intermediate size with some apparent structure despite the merging.
