The galaxy presents as a centrally concentrated, relatively smooth object. It appears elliptical in shape, exhibiting a high degree of radial symmetry. There is a gradual decrease in surface brightness from the core outwards. The central region exhibits a bright, almost stellar-like nucleus. The overall color gradient transitions from a bluer hue in the core to a more reddish or neutral color in the outer regions, suggesting a potential mix of stellar populations, with younger, hotter stars concentrated towards the center and older, cooler stars dominating the outskirts. There is no discernible spiral structure or prominent dust lanes. The galaxy's overall smooth and rounded appearance suggests a lack of significant recent merger activity or major disturbances. Faint, diffuse light extends beyond the main body of the galaxy, forming a faint halo.
