The galaxy exhibits an elongated, cigar-like morphology. Its overall structure appears relatively smooth with a slight hint of a disk component. A small portion of the galaxy at the bottom appears somewhat disturbed, as if experiencing minor gravitational interactions, or some star-forming activity. There is a prominent color gradient, shifting from bluer hues at the top to redder tones at the bottom. This may indicate a gradient in stellar population or dust content across the galaxy, with younger stars and/or less dust towards the top. The estimated size of the galaxy is moderate. The overall appearance suggests a system undergoing a period of transition in its evolution.
