The galaxy appears to be an elongated, disk-shaped system, viewed nearly edge-on. It exhibits a concentrated central bulge, brighter and yellower in color than the surrounding disk. The disk itself shows some evidence of structure, though the resolution is limited. Fainter, bluer regions are visible along the outer edges of the disk, potentially indicating areas of more active star formation. The overall color suggests a mix of older stellar populations in the bulge and younger stars in the disk. There is no strong evidence of a major ongoing merger or tidal disruption, although minor disturbances cannot be ruled out. The galaxy presents a relatively smooth appearance, indicating an evolved and settled morphology. The estimated size of this galaxy would make it one of significant size.
