The galaxy presents as an elongated, cigar-shaped object with a distinct central bulge. There is a disk component that appears somewhat inclined relative to the line of sight. The central region exhibits a yellowish hue, indicative of an older stellar population. The outer edges show a bluer color, possibly suggesting ongoing or recent star formation. The disk is not uniformly bright; there appear to be some subtle variations in luminosity across its extent. Overall the galaxy exhibits a relatively smooth profile, with no prominent signs of major disturbances or mergers.
