The galaxy presents as a roughly elliptical, somewhat diffuse object. The central region exhibits a notably brighter, more concentrated luminosity, suggesting a prominent galactic nucleus. A faint, extended halo appears to surround the central region, though its boundaries are ill-defined, hinting at a possible gradual decrease in stellar density outwards from the core. The overall color appears relatively homogenous across the galaxy, though some subtle variations in hue are detectable, with the core appearing to contain some bluer light. The galaxy doesn't present any easily detectable spiral arm structure or clear signs of significant tidal disruption.