The galaxy exhibits a pronounced disk structure, oriented approximately edge-on relative to our line of sight. Spiral arm features are discernible, though somewhat obscured by the viewing angle. Evidence of a central bar is apparent, extending through a significant portion of the galactic center. The central bulge appears moderately sized, contributing substantially to the overall luminosity. The galaxy shows a mix of smooth and featured morphology, suggesting a transition phase in its evolutionary state. Overall, the object exhibits a slightly disturbed morphology which could indicate minor gravitational interactions or recent accretion events. The color distribution suggests ongoing star formation, with bluer regions likely indicating areas of active star birth. The size of the galaxy seems to be of an average spiral galaxy.
