The galaxy presents an elliptical morphology, elongated along a major axis. Its core exhibits a high surface brightness, appearing nearly uniform in color, indicative of an older stellar population. The outer regions of the galaxy gradually decrease in luminosity, displaying a smooth transition from the core to the surrounding space. There is a subtle color gradient within the galaxy, with the core appearing slightly yellower, suggesting a concentration of older stars. Faint asymmetry is observed in the lower left section of the galaxy, which could indicate minor tidal disruption or recent interaction. Despite this, the primary structure appears largely undisturbed, indicative of a relatively relaxed system.
