The galaxy presents as an edge-on spiral system. A prominent dust lane is not readily apparent, though a slight obscuration may be present along the equatorial plane. The central bulge appears to be quite extended, displaying a near-elliptical morphology, possibly with a rounded profile. The luminosity of the bulge is significant, indicating a potentially large population of older stars. A faint, diffuse halo is visible around the bulge, possibly indicating the presence of a substantial stellar population. The disk appears relatively thin and elongated. Faint disk features could suggest star formation regions, but resolution limitations preclude definitive identification. There does not appear to be evidence of a significant merger or major disturbance in the galaxy's morphology; the disk is relatively undisturbed. The integrated color suggests a population mix of younger, bluer stars and older, redder stars. 
