The galaxy presents as a lenticular or early-type spiral galaxy, with a significant spheroidal component dominating its structure. It exhibits a smooth, centrally concentrated light distribution, with a noticeable bulge region. There is a slight elongation, suggesting it is not perfectly spherical. The galaxy displays a color gradient, with the central region appearing more yellow/orange, indicative of an older stellar population, while the outer regions exhibit a bluer hue, possibly indicating younger stars or some star formation, though not vigorous. No prominent spiral arms or dust lanes are clearly visible; any disk-like component appears to be smooth and featureless. There are no signs of ongoing major mergers or significant tidal disturbances. The overall morphology suggests a relatively evolved system.
