The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology. The light distribution suggests a concentrated central region, with a gradual decrease in luminosity extending outwards. The galaxy exhibits a roughly intermediate ellipticity, not appearing perfectly spherical, nor highly elongated, presenting more of a slightly ovoid shape. No prominent spiral arm structures or disk-like features are discernible. There is no clear indication of any ongoing major merger events, although subtle asymmetries or minor disturbances cannot be entirely ruled out. The galaxy's color appears to be dominated by blue and green, which might indicate a relatively old stellar population with minimal ongoing star formation. This general color is consistent throughout the galaxy.
