The galaxy presents as an edge-on disk galaxy with a prominent bulge. The central bulge exhibits a yellowish hue, suggesting an older stellar population with minimal ongoing star formation. The disk appears relatively smooth, lacking prominent spiral arm structures. The light distribution within the disk gradually diminishes from the bulge towards the outer edges. There is a subtle color gradient across the disk, potentially indicative of differences in stellar populations or dust content. The overall morphology suggests a well-developed and relatively quiescent galaxy.
