The galaxy presents a predominantly smooth morphology, with a slight elongation. The central region exhibits a concentrated luminosity, appearing nearly spherical and yellow, suggesting an older stellar population. Faint disk-like features are visible extending outwards from this central bulge. The overall color is weighted towards the redder end of the spectrum. No pronounced spiral arm structure is observed. There appear to be some minor disturbances in the outer disk, but no strong indications of a major merger event are visible.
