The galaxy presents as a lenticular or possibly an elliptical type, displaying a smooth, centrally concentrated luminosity profile with a noticeable lack of distinct spiral arm structures. The galaxy exhibits a moderate elongation and a slightly cigar-shaped morphology. The color gradient suggests a relatively older stellar population, as indicated by the yellowish hue of the galactic bulge. There is a small indication of minor disturbances to the galaxy, though it appears mostly undisturbed, not presenting any signs of ongoing or recent major mergers. 
