The galaxy exhibits a disk-like morphology, though the image resolution limits detailed analysis of spiral arm structure. The central bulge appears prominent and has a yellowish hue, indicative of an older stellar population. The disk, while somewhat blurred, displays bluer tones suggesting regions of ongoing star formation. The galaxy is not perfectly circular, displaying an elongated shape reminiscent of a cigar. There are possible signs of minor gravitational disturbances with slightly asymmetrical disk features. Overall, the galaxy presents a system exhibiting characteristics of both smooth elliptical galaxies and galaxies with disks, implying a possible transition or past interaction phase.
