The galaxy presents as a relatively smooth, elliptical morphology. Its light is centrally concentrated with a radial falloff, showing no obvious spiral arm structure or prominent disk features. The galaxy exhibits a nearly round shape with only slight elongation. There appears to be a homogeneous color distribution within the galaxy, suggestive of an older stellar population. There is no evidence of significant dust lanes or recent star formation activity. The galaxy appears isolated, showing no strong indications of tidal interactions or ongoing mergers with other galaxies, although a minor disturbance cannot be ruled out.
