The galaxy presents as a centrally concentrated, elliptical system. It exhibits a smooth, diffuse morphology with no readily discernible spiral arm structure or prominent dust lanes. The galaxy's color profile is predominantly red/yellow, suggesting an older stellar population with reduced ongoing star formation. The overall shape appears nearly circular, though a slight elongation cannot be ruled out based on the available imagery. There is no obvious evidence of tidal features or ongoing major mergers, although minor disturbances are possible. The light distribution indicates a high degree of symmetry and a gradual decline in brightness from the core outwards.
