The galaxy exhibits a generally smooth, elongated morphology, appearing somewhat cigar-shaped. The light distribution is concentrated towards the center, with a noticeable bulge that displays a yellowish hue, potentially indicating an older stellar population. The outer regions are less defined, with a bluer tint, possibly suggesting the presence of some younger stars and ongoing, though limited, star formation. There may be some minor disturbances in the disk, but no clear evidence of major mergers or significant interactions. The galaxy is primarily a smooth system.
