The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution appears largely homogenous with no obvious spiral arm structures or distinct features. There is a slight elongation in its overall shape, exhibiting a deviation from perfect circularity, with an apparent deviation towards a more elliptical morphology. The color profile suggests a population of older stars. The central region shows a slight reddening, implying a greater density of older stellar populations. The outer regions appear slightly bluer, suggestive of a small population of younger stars and, subsequently, ongoing but limited star formation. There is no evidence of any major ongoing or recent mergers. The galaxy may have experienced minor disturbances due to the slight asymmetry.
