The galaxy appears to be a relatively small, edge-on spiral or lenticular galaxy. It exhibits a smooth, elongated morphology with a bright, concentrated central bulge. There's a subtle hint of a disk component extending outwards from the bulge. Coloration suggests moderate star formation, implied by the presence of some blue hues particularly within the disk area. The shape is elongated, with a high ratio of major to minor axis, indicating a flattened structure when viewed at this angle. There is no strong evidence of recent mergers or major disturbances in the overall structure, though subtle irregularities cannot be ruled out due to the image resolution. The galaxy is relatively isolated.
