The galaxy presents as a largely smooth, centrally concentrated object. It exhibits an elliptical morphology with a pronounced bulge and a slight elongation, leaning towards a cigar shape. A faint blue hue pervades the galaxy's central region, suggesting the presence of a younger stellar population compared to the rest of the galaxy, though this area also exhibits signs of older stars as well. Fainter outer regions can be observed. There is a small amount of asymmetry, possibly suggesting the presence of minor disturbances or an ongoing interaction with a smaller companion, though it does not seem like the galaxy is undergoing a major merger. Star formation rates appear to be relatively low.
