The observed galaxy presents as a spiral galaxy, viewed at a steep inclination nearing edge-on. The galactic bulge appears centrally located and exhibits a yellowish hue, suggesting a population of older stars. Faint spiral arms are visible extending from the central bulge. The spiral arms are difficult to discern due to the inclination, but appear tightly wound. No apparent bar structure is detectable in the central region. The disk demonstrates clumpy areas, indicating the presence of active star formation regions. The overall color of the disk exhibits a bluish tint, indicating the presence of younger, hotter stars. There is no evidence of major mergers or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed.
