The galaxy presents a moderately elliptical morphology. Its central region exhibits a smooth, concentrated luminosity, appearing yellowish-orange, potentially indicative of an older stellar population. Surrounding the core, there's a less concentrated, greenish-blue halo. This halo could suggest the presence of younger, hotter stars and/or ionized gas. The overall structure appears relatively undisturbed, with a slight hint of asymmetry to the lower left, but lacking strong evidence of ongoing major mergers or tidal interactions. Based on its apparent color gradient and smooth central region, the galaxy is possibly an early-type spiral galaxy.
