The galaxy presents as an elongated, disk-like structure seen at an oblique angle, not quite edge-on, but significantly inclined from face-on. The central region appears brighter and more concentrated, suggesting a prominent galactic bulge. This central region exhibits a yellowish-white hue, indicative of an older stellar population, which is common for galactic bulges.

Fainter and less concentrated disk is bluer in color, suggesting the presence of younger, hotter stars and active star formation. The outer edges of the disk appear somewhat diffuse and irregular, hinting at possible interactions or recent accretion events. There's a slight asymmetry to the overall shape, possibly indicating a minor gravitational disturbance. Overall, the galaxy is relatively compact with a well-defined structure.
