The galaxy presents an elongated morphology, potentially a disk-like structure viewed at an oblique angle. The central region exhibits a brighter, more concentrated luminosity profile, suggesting a bulge or a higher density of stars and/or gas. The galaxy appears to possess a relatively smooth texture overall, with hints of irregularities or disturbances in the disk region. There is evidence of bluer hues distributed throughout the galaxy, indicative of ongoing star formation. These regions are not sharply defined but show a more diffuse distribution. Faint features, possibly tidal tails or disrupted spiral arms, might be present but are not distinctly visible.
