The galaxy presents as a smooth, elliptical-like structure with a notable central bulge. It exhibits a generally featureless morphology, with a relatively high degree of central concentration and a gradual decrease in surface brightness outwards. The core region appears significantly brighter and exhibits a yellow-white hue, likely indicating a population of older stars. The outer regions of the galaxy are more diffuse and have a slightly reddish tint, suggestive of a different stellar population or dust content compared to the core. There is very little evidence of spiral arms or prominent dust lanes, and the overall structure suggests a system that is relatively relaxed and evolved. The apparent ellipticity indicates some degree of flattening, though the galaxy does not present as a highly flattened disk system. There is no obvious sign of any recent or ongoing major merger events, however minor disturbances cannot be ruled out.
