The galaxy presents as a fairly smooth, centrally concentrated light distribution. There's a slight elongation, leaning toward an in-between elliptical shape rather than perfectly round or cigar-shaped. The color profile suggests a relatively evolved stellar population, with a yellowish-orange hue dominating the central regions, indicating the presence of older, cooler stars. No distinct spiral arms or prominent dust lanes are visible; the overall structure appears largely featureless, which may indicate a relatively quiescent or post-starburst evolutionary phase. There is no apparent evidence of an ongoing major merger event, though the presence of a minor disturbance cannot be ruled out given the subtle asymmetry in the light distribution.
