The galaxy presents as an elliptical morphology, exhibiting a generally smooth structure without prominent spiral arms or a distinct disk. The central region is characterized by a high concentration of light, suggesting a substantial stellar population. The galaxy appears moderately bright, with a color profile that indicates a mixed stellar population, possibly with some ongoing or recent star formation. The galaxy's shape appears somewhat in between round and elliptical. There are no obvious signs of any major mergers or significant tidal disturbances.
