The galaxy presents as a generally smooth object, with an overall rounded morphology. The light distribution appears relatively uniform, although there is a suggestion of a slight elongation. The central region exhibits a higher surface brightness, indicative of a bulge. There is evidence of a potential companion galaxy or tidal feature located nearby. The color profile suggests a population of older stars. The limited presence of distinct features or spiral arms implies a relatively low star formation rate. There are no signs of major mergers occurring.
