The galaxy presents as a primarily smooth, centrally concentrated object. Its overall shape is somewhat elliptical, exhibiting a slight elongation. The core region is bright and yellowish, indicating a likely concentration of older stellar populations. A bluer, fainter halo surrounds the core, suggesting the presence of younger stars or ongoing star formation, though at a relatively low rate. There is no obvious evidence of spiral arm structures or significant dust lanes. The galaxy does not appear to be undergoing any major merging events, although there may be some minor disturbances in its outer regions.
