The galaxy presents a distinctly elongated, cigar-like morphology. It exhibits a predominantly smooth structure with a notable absence of defined spiral arms or prominent dust lanes. The central region displays a concentration of light, suggesting a possible bulge or nucleus. The overall color appears reddish, potentially indicating an older stellar population and/or significant dust obscuration. There is a small feature located on the side of the galaxy that may be some form of a disturbance. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major merging activity in the immediate vicinity.
