The galaxy presents as a largely featureless, elliptical morphology with a smooth light distribution. A dominant central bulge is apparent, characterized by a concentrated, yellow hue indicative of an older stellar population. The overall shape is approximately round. There is little evidence of spiral arms or a pronounced disk structure. Some slight asymmetry or distortion is noted in the outer regions, potentially indicating minor interaction or tidal disturbance with a nearby galaxy. The galaxy appears relatively isolated in this field.
