The galaxy presents an elongated, disk-like morphology, viewed nearly edge-on. There is a prominent central bulge region displaying a yellowish hue, suggesting an older stellar population dominating this area. The disk is characterized by a bluer color gradient away from the central bulge, indicative of more recent or ongoing star formation. The distribution of light appears somewhat disturbed or irregular within the disk, potentially suggesting ongoing merger activity or tidal interactions. There are also some fainter star-forming regions present that display a much more green/blue color. Overall, the galaxy is actively forming stars, although it is not at a particularly high rate. The estimated size of the galaxy is on the larger size. There is some visible dust obscuring the inner regions of the disk.
