The galaxy appears as a disk galaxy, seen nearly edge-on. The central bulge is prominent and exhibits a yellowish-white hue, indicating an older stellar population. A faint, extended disk is visible surrounding the bulge. The disk appears relatively smooth, with no apparent spiral arm structure visible in this image. There is a slight color gradient from the center to the edges, with the outer regions appearing somewhat bluer, suggesting the presence of younger stars or ongoing star formation. The overall morphology suggests a relatively quiescent galaxy with moderate stellar mass. There is no evidence of a recent major merger or significant tidal disturbances.
