This galaxy presents a generally smooth appearance, although subtle features are discernible. The central region exhibits a bright, concentrated core, surrounded by a fainter, more diffuse halo. The light distribution appears roughly elliptical, with a slight elongation suggesting a disk-like component viewed at a shallow inclination. There are hints of minor disturbances or asymmetries in the outer regions, possibly indicative of past interactions or mergers. The galaxy's color is primarily blue-white, suggesting a population of relatively young, hot stars, especially in the inner region. Fainter, redder regions can also be observed, which may indicate the presence of older stars or dust lanes. There is no single obvious feature such as a spiral arm or bar.
