The galaxy presents a predominantly smooth morphology, appearing as a lenticular or early-type spiral galaxy viewed at a significant inclination. The central bulge is prominent and exhibits a yellowish hue, indicative of an older stellar population. Moving outward from the bulge, a flattened disk is observed. While the disk lacks distinct spiral arm structure, there are subtle variations in color and brightness, suggesting regions of ongoing, albeit subdued, star formation. The disk appears elongated, giving the galaxy a cigar-like shape. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity of the galaxy, although some minor disturbances cannot be ruled out. The overall light distribution is centrally concentrated, decreasing gradually towards the edges of the disk.
