The galaxy presents an elongated morphology, suggesting a disk-like structure viewed at an oblique angle. A prominent central bulge is apparent, exhibiting a concentrated luminosity profile. The color gradients across the galaxy indicate variations in stellar populations. The bluish hues at the extremities are suggestive of ongoing star formation activity. The internal structure appears disturbed, which may be indicative of recent or ongoing interactions with another galaxy. Faint extensions or tidal features are visible, further suggesting gravitational disturbances. Overall, the galaxy displays characteristics consistent with an intermediate-type spiral galaxy undergoing some form of interaction or merging activity, likely resulting in enhanced star formation.
