The galaxy appears to be a relatively bright, disk-shaped system, seen at an oblique angle. A central bulge is prominent and appears smooth, exhibiting a yellow-orange hue. The disk component shows a bluer tint, and the overall morphology suggests it is a spiral galaxy, although the spiral arms are not well-defined. The galaxy displays some degree of internal structure, though details are limited. It appears to be relatively isolated, with no obvious signs of major interaction or merging activity visible in this image. The roundness of the object suggests it is not cigar shaped, but is in between round and cigar shaped. There might be some minor disturbances of a merging event occurring. The low star formation rates and high mass suggest that this is an older galaxy.