The galaxy presents as a moderately luminous, relatively compact object. Its overall morphology appears largely smooth and spheroidal, exhibiting a high degree of central concentration. The color profile suggests a mixture of stellar populations, with a central region displaying a slightly bluer hue transitioning to a more uniform color in the outer regions. There is little indication of distinct spiral arms or other prominent features. The overall structure is consistent with an early-type galaxy, likely an elliptical or lenticular type. The smooth appearance indicates that there is no significant on-going merger activity. The galaxy is relatively isolated.
