The galaxy appears as a single, concentrated luminous object. Its morphology is predominantly smooth and elliptical, displaying a high degree of central concentration. The light profile decreases uniformly from the core, with no evidence of spiral arms or a prominent disk structure. The color gradient suggests a relatively evolved stellar population, with the inner region exhibiting a warmer, yellower hue compared to the outer regions, which appear slightly redder. There is no clear indication of ongoing major star formation or significant dust lanes. Faint asymmetry may be present, but the galaxy is mostly undisturbed, with no signs of recent major merger activity.
