The galaxy presents as a spiral, viewed at a significant angle. The central bulge exhibits a concentrated, bright, yellow-white hue, suggesting a high density of older stars. The galactic disk is visible, though not sharply defined. It shows hints of spiral arm structure. The spiral arms are subtly bluer than the central bulge, implying the presence of younger, hotter stars and ongoing star formation. A degree of morphological disturbance appears to be present, perhaps a mild tidal effect due to gravitational interaction with another galaxy. One side shows an additional feature that could be either a tidal tail or an area of enhanced star formation.
