The galaxy presents an elongated morphology, appearing somewhat flattened, suggesting a disk-like structure viewed at a moderate inclination. The central region exhibits a bright, concentrated bulge, yellowish-white in color, indicating a population of older, evolved stars. Extending outwards from the bulge, a fainter, bluer disk is discernible. This disk displays mottled texture, potentially indicative of spiral arm structures or areas of active star formation. The blue hue suggests the presence of younger, hotter stars within these regions. There are some slight irregularities in the shape of the disc, it is possible the galaxy is undergoing or has undergone a minor merger. Overall, the galaxy shows a complex structure with a combination of old and young stellar populations.
