The galaxy presents as a relatively smooth, centrally concentrated object with a noticeable radial color gradient. The central region exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color shifts towards a bluer tint, possibly indicating younger stellar populations or ongoing star formation in the outer regions. The galaxy appears nearly circular, indicating a low degree of apparent flattening. No prominent spiral arms or bar structures are discernible. There is a slight indication of subtle disturbances within the galaxy structure, but no major mergers or tidal features are evident. The relatively smooth appearance suggests that this galaxy could be a spheroidal or elliptical galaxy.
