The galaxy presents as a somewhat elongated, disc-like structure with a noticeable central bulge. The color is primarily a yellowish-orange hue, suggesting an older stellar population. The smooth appearance indicates a relatively evolved system, with signs of past or ongoing star formation, though at a moderate rate. There are hints of internal structure, possibly spiral arms or dust lanes, but these are not sharply defined. The galaxy appears relatively isolated, without obvious signs of major interactions or mergers, though there may be minor disturbances present in its morphology. The overall shape is somewhat cigar-like, indicating it is not perfectly circular.
