The galaxy appears to be a relatively smooth, centrally concentrated object. There is a noticeable radial gradient in surface brightness, with a bright, unresolved core that fades into a more diffuse halo. The overall shape is somewhat elliptical, but not significantly elongated. Based on color, the central regions appear bluer than the outer regions, which are more red. There is no apparent spiral structure, bar, or dust lane visible at this resolution. There is no strong evidence of any major ongoing merger activity or tidal disturbances, although a slight asymmetry can be noticed on the right side of the galaxy, possibly indicating a minor interaction.
