The galaxy presents as an elliptical morphology, though not perfectly spherical. It appears somewhat elongated, with a major axis slightly exceeding its minor axis.

The light distribution across the galaxy is not uniform. The central region displays a brighter intensity, suggesting a denser concentration of stars or possibly an active galactic nucleus, though the resolution is insufficient to confirm the latter. The intensity gradually decreases outwards from the center, characteristic of elliptical galaxies.

The color profile indicates a generally older stellar population. The galaxy exhibits reddish hues overall, which are most notable in the periphery. Bluer color is concentrated in what appears to be a bright knot. This may be due to local, more recent, star formation activity.

There is evidence of possible tidal features or disturbances. Irregularities in the outer regions hint at gravitational interaction with another galaxy. The overall morphology suggests an ongoing or recent merging event. Patches of nebulosity, if present, are below the resolution threshold for reliable identification.
