The galaxy presents a generally smooth morphology, appearing largely spheroidal. The light distribution is centrally concentrated, with a noticeable decline in intensity towards the outer regions. There is a subtle deviation from perfect roundness, appearing slightly elongated. Visual inspection reveals a dominant, centralized bulge. Faint, diffuse features are noted, suggesting potential minor disturbances or interactions. There are subtle hints of possible underlying disk structures, but the smoothness suggests the bulge dominates the galaxy's overall appearance. Star formation appears to be present, at least at low levels.