The galaxy presents as a somewhat elongated, disk-shaped object with a noticeably bright central bulge. The light from the bulge appears yellowish, suggestive of an older stellar population. The disk component exhibits a bluish tint, indicating the presence of younger, hotter stars and possibly ongoing star formation. There may be indications of spiral arm structure within the disk, though the resolution limits clear identification. Overall, the galaxy exhibits a moderately inclined orientation relative to our line of sight, lending it the slightly cigar shaped appearance. The edges of the disk fade smoothly into the background sky.
