The galaxy presents as a moderately luminous, relatively smooth object. Its shape is generally elliptical, tending towards round rather than significantly elongated. A central bulge is apparent, exhibiting a yellowish-orange hue, suggesting a population of older stars. Surrounding the bulge, there is a diffuse halo with a bluish tint, potentially indicative of some ongoing star formation. The overall structure appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. The galaxy appears to be a fairly massive system, and low rates of star formation are observed within the structure. 
