The galaxy presents an elongated, cigar-shaped morphology. There is a smooth appearance with a concentration of light towards the central region, indicative of a bulge. A disk structure appears present and is oriented edge-on. The central region exhibits a reddish hue, which may be due to a high concentration of older stars or dust obscuration. The outer regions of the galaxy display bluer colors, possibly signifying younger stellar populations and ongoing star formation. There are very minor signs of tidal disturbances, suggesting a relatively undisturbed recent history and negligible signs of any recent mergers. 
