The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in luminosity towards the outer edges. There is a noticeable lack of spiral arm structure or prominent dust lanes. The galaxy is relatively round in appearance, without significant elongation. Faint disturbances in the outer regions could indicate minor past interactions or mergers, but are not overtly apparent. The galaxy exhibits a color gradient, transitioning from a more yellow hue at the core to slightly redder tones in the halo, suggestive of an older stellar population dominating the central regions with younger stars populating the outer regions.
