The galaxy presents as a spiral with a prominent central bulge exhibiting a yellowish hue, suggestive of an older stellar population concentrated in that region. Fainter spiral arms extend outwards from the bulge, showing bluer tones, potentially indicating regions of active star formation. The arms do not appear tightly wound, giving the galaxy a less defined spiral structure. There's some indication of mild disturbance in the arm structure, but no clear evidence of a major ongoing merger. The disk is viewed at an angle, not quite edge-on, allowing some view into the spiral structure. A moderate bulge is visible. No strong bar is readily apparent in the galactic center, and no interactions with other galaxies are obviously visible. Overall, the galaxy appears as an average-sized spiral at a significant distance, and is relatively undisturbed.
