The galaxy appears to be a spiral galaxy viewed nearly edge-on. There is a prominent central bulge, exhibiting a rounded morphology. The disk is distinctly visible and oriented horizontally across the image. Due to its near edge-on orientation, internal structures within the disk, such as spiral arms and dust lanes, are not readily discernible. The galaxy displays a reddish-orange hue, suggesting a population of older stars and a lower rate of current star formation. There is no obvious evidence of a major ongoing merger or tidal disruption. A slight asymmetry may indicate a minor gravitational disturbance, but this cannot be confirmed without further data. The galaxy appears relatively smooth in overall structure.
