The galaxy presents as a moderately inclined spiral or lenticular galaxy. It exhibits a diffuse, centrally concentrated bulge. The bulge region appears largely smooth with a hint of redder light in the inner regions, suggestive of an older stellar population. The disk component is less prominent and shows a bluer hue, possibly indicative of ongoing star formation. The overall shape is elliptical with a hint of distortion, suggesting a possible interaction or past merger event. There are subtle hints of asymmetry. The galaxy appears relatively isolated with no obvious companion galaxies in close proximity.
