The galaxy presents as a relatively smooth, featureless object. Its shape is elongated, appearing somewhat cigar-shaped rather than perfectly round. The central region exhibits a higher surface brightness, suggesting a concentration of stars and possibly a galactic bulge. There is a noticeable color gradient, with the core appearing more yellowish-white, transitioning to a bluer hue towards the outer edges. This color variation could imply older stellar populations concentrated in the core, with younger, bluer stars populating the galactic disk. No signs of active merging or major tidal disturbances are readily apparent.
