The galaxy presents as an elongated, cigar-shaped structure. It exhibits a central, brighter core, potentially indicating a concentration of older stars or a possible active galactic nucleus. The light is blueish in the central area, potentially indicating star formation. There are traces of dusty material. A faint, extended halo surrounds the main body of the galaxy, exhibiting a bluer hue which might imply younger stars and more recent or ongoing star formation within its outer regions. Overall, it appears to be a disk galaxy viewed at a high inclination with respect to our line of sight. There is a very faint structure extending from the galaxy which may be an interacting galaxy or a star forming tidal tail.
