The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. There is a prominent central bulge with a concentrated luminosity. The bulge appears smooth with no distinct features. The disk component exhibits a gradient in color, suggestive of differing stellar populations or dust obscuration. Near the central bulge, the color appears more yellow/red, potentially indicating an older stellar population. Progressing outward from the bulge, the color appears slightly bluer. The disk appears relatively smooth, lacking apparent spiral arm structures or prominent star-forming regions. Overall, the galaxy’s morphology suggests a relatively quiescent system with minimal current star formation. There is no evidence of ongoing mergers or tidal disturbances in the immediate vicinity.
