The galaxy presents as an elliptical morphology, elongated along its major axis. A smooth, centrally concentrated bulge dominates the structure, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Fainter, diffuse blueish light extends from the bulge along the major axis, potentially indicating the presence of a relatively faint disk component with some ongoing star formation. There are no obvious spiral arm features. Overall, the galaxy appears relatively undisturbed, with no signs of major mergers or tidal disruptions.
