The galaxy presents as a relatively compact object with a discernible, albeit faint, disk-like structure. The overall color is suggestive of a mature stellar population, with a somewhat redder central region possibly indicating an older population of stars concentrated towards the core. There are hints of bluer regions within the disk, possibly indicative of younger star formation. The galaxy is not perfectly circular; it has a slightly elongated, cigar-like appearance. There seems to be some form of gravitational disturbance acting on the galaxy, though it is hard to say exactly how major it is. It's also possible that this is a merging galaxy.
