The galaxy presents as a significantly inclined, likely spiral, system. A prominent central bulge, appears yellowish, indicating an older stellar population. A flattened disk extends outward from the bulge, displaying a bluer hue indicative of younger stars and ongoing star formation, although at a modest rate. The disk is relatively smooth in appearance, with possible faint spiral arm structures difficult to resolve due to the inclination. There is no obvious sign of a strong bar feature or major merger event, though some minor disturbances or tidal features cannot be entirely ruled out. The galaxy is estimated to have a stellar mass of approximately 10^10.9 solar masses.
