The galaxy presents as a somewhat elongated, luminous structure with a central bulge. There is evidence of a disk-like component, though its features are not sharply defined. The primary color of the galaxy appears to be bluish-white, particularly in the central region, suggesting a population of younger, hotter stars. Fainter, reddish regions are scattered throughout the galaxy, potentially indicating areas of active star formation or older stellar populations. There may be slight disturbances visible, indicating possible minor interactions.
