The galaxy presents as a largely featureless, elliptical-like structure with a concentrated central bulge. It is characterized by a smooth, diffuse light distribution, lacking prominent spiral arms or distinct dust lanes. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue in the central region, gradually fading to a bluer color in the outer regions of the halo. The outer edges appear to be relatively uniform in color, and there is no apparent evidence of significant tidal disturbances or ongoing major merger events. The galaxy's morphology suggests that it has undergone significant evolution, likely resulting in the observed smooth and spheroidal shape. A slight distortion in the halo suggests possible minor tidal interactions.
