This galaxy presents as a relatively compact, disk-shaped object with evidence of significant ongoing disturbances to its morphology. The central bulge is moderately sized, exhibiting a somewhat elliptical profile with a major axis oriented approximately north-south. The disk component displays an uneven distribution of light, indicating possible interactions or recent merger events. There is evidence of tidal tails or distorted spiral arm structures extending away from the main body of the galaxy, especially towards the north and perhaps extending away from the opposite side of the disk as well. These extensions are diffuse and appear less structured than typical spiral arms. Star formation appears moderately active throughout the galaxy, with a notable concentration of blue-shifted light in the central region and in some of the disturbed disk features. The overall color of the galaxy suggests a mix of older stellar populations in the bulge and younger, star-forming regions within the disk and tidal features.
