The galaxy presents as an elongated, disk-shaped structure, likely a spiral or lenticular galaxy viewed at a high inclination. The central bulge appears yellowish, suggesting an older stellar population. The disk shows a faint bluish tint along its edges, potentially indicative of younger stars and ongoing star formation. A distinct red patch appears at one end of the galaxy, possibly indicating a region of intense star formation or dust obscuration. The overall appearance is smooth, with no obvious signs of major disruption or interaction with other galaxies, though minor disturbances cannot be ruled out. The elongated shape suggests a non-negligible rotational velocity. The galaxy is relatively faint, yet clearly defined against the background.
