The galaxy presents an elongated morphology, suggestive of a disk-like structure viewed at a significant inclination. The central region exhibits a high concentration of luminosity, indicating a prominent galactic bulge or nucleus. A diffuse, extended halo surrounds the brighter core, gradually fading into the background. There appears to be some patchy structure within the disk, with potential evidence of spiral arm segments or dust lanes. A distinct, compact luminous region is observed at the edge of the galaxy, potentially indicating an area of active star formation. There is also evidence of a slight disturbance in the morphology of the galaxy suggesting it may be undergoing a minor merger. The color profile exhibits variations, possibly related to differences in stellar populations or dust obscuration across the galaxy.
