The object is a galaxy exhibiting characteristics of both a smooth, elliptical structure and a disk galaxy. The central region displays a concentrated, smooth morphology, suggesting a significant bulge component. A faint, disklike structure extends horizontally from this bulge. The disk appears somewhat irregular, with a mottled texture. The disk appears to be more concentrated near the center. There also appears to be a faint arm or feature that is interacting or emerging from the disk. There may be evidence of possible tidal features or minor disturbances, possibly related to past or ongoing interactions with another galaxy. The galaxy displays a color gradient, transitioning from a more reddish hue in the center to a slightly bluer tone towards the outer edges of the disk. This color variation could indicate differences in stellar populations, with older, redder stars concentrated in the bulge and younger, bluer stars residing in the disk. The galaxy appears to be actively merging with another galactic body.
