The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The core exhibits a bright, yellowish hue, potentially indicative of an older stellar population dominating the central region. A fainter, slightly bluer halo surrounds the core, which may suggest the presence of a younger stellar population in the outer regions. There is a slight indication of asymmetry, possibly a minor disturbance, but no clear evidence of strong spiral arm structure or a major merger event. Overall, the galaxy appears to be transitioning, with star formation still actively occurring, but at a relatively subdued rate.
