This galaxy presents as a relatively compact, disk-shaped structure. The central region exhibits a brighter, more concentrated luminosity profile, suggesting the presence of a significant galactic bulge. The galaxy's disk appears subtly inclined, with an intermediate viewing angle, allowing for a partial view of its spiral structure. Faint, diffuse spiral arms emanate from the central bulge, displaying hints of ongoing star formation, but the overall arm structure is somewhat flocculent. There is an apparent distortion present, possibly due to a minor tidal interaction. In the periphery of the disk, a small, reddish area may indicate a region of older stars, obscured by dust, or a separate, interacting object. The galaxy's color indices suggest that it is a relatively quiescent system with a low star formation rate, but it still exhibits some regions of active star birth.
