The galaxy presents a moderately elliptical morphology. Its central region exhibits a bright, concentrated core, suggestive of a substantial bulge component. The light profile appears relatively smooth, with a noticeable falloff in intensity from the core outwards. The overall color is yellowish-white, which could indicate an older stellar population dominating the light output. Hints of bluer color appear on the edges of the galaxy. There is no obvious presence of spiral arms or significant dust lanes and no evidence of a recent or ongoing major merger event, though the slight asymmetry might indicate minor disturbances or interactions.
