The galaxy presents as a moderately elongated, lenticular or early-type spiral system. It displays a relatively smooth, centrally concentrated luminosity profile, indicative of an older stellar population. The dominant colour is a yellowish-orange hue, consistent with a lack of significant ongoing star formation and a predominance of evolved stars. There are no discernible spiral arm structures or prominent dust lanes. The overall morphology suggests a relatively quiescent system, possibly transitioning towards a more elliptical shape.
