The galaxy presents as a relatively smooth, elongated object. Its morphology suggests a cigar-shaped structure. There's a distinct color gradient, with the central region appearing more reddish in hue, possibly indicative of an older stellar population or dust obscuration. The outer regions exhibit a bluer tint, which could suggest ongoing star formation, but it is faint. No distinct spiral arm structure or prominent features such as star clusters or dust lanes are immediately apparent. Overall, the galaxy appears undisturbed, with no signs of major mergers or tidal disruptions.
