The galaxy presents a distinctly elongated, cigar-shaped morphology. Its light profile appears relatively smooth overall, but with subtle irregularities that suggest the presence of some internal structure. A brighter, somewhat amorphous central region is observed, possibly indicative of a bulge or a concentration of older stars. The outer regions of the galaxy are fainter and appear diffuse, gradually fading into the background. The color gradient across the galaxy appears subtle, transitioning from slightly bluer hues in the outer regions to subtly redder tones toward the central area, hinting at variations in stellar populations or dust content. No obvious spiral arms or strong star-forming regions are readily discernible. There is a hint of minor disturbance in its overall form, perhaps due to an interaction with another galaxy.
