The galaxy presents as a centrally concentrated system with a generally smooth morphology. The central region exhibits a bright, slightly elongated core. The light distribution falls off gradually from the center, displaying a somewhat elliptical shape. There is a hint of a disk-like structure, with some faint, diffuse features extending outwards. The galaxy appears to be a mature system, likely an elliptical galaxy, with ongoing but relatively low levels of star formation. There may be some minor tidal disturbances, indicating potential past interactions with other galaxies, but not indicative of a major merger.
