The galaxy exhibits a somewhat elongated morphology, suggesting a disk-like structure viewed at an oblique angle. The light distribution appears relatively smooth, with a concentration of luminosity toward the center. The color gradient transitions from a slightly bluer hue in the outer regions to a more yellow or red tone towards the core. There is a possible hint of some spiral arm structure. No obvious dust lanes are visible. There is no clear evidence of a bulge component. Overall, the galaxy appears to be a relatively low mass system.