This galaxy exhibits a distinct elongated, cigar-shaped morphology. The central region displays a relatively smooth texture with a bright, concentrated core, suggestive of a large amount of stars congregated in that area. The core has a slightly red hue to it, possibly indicating an older stellar population. Moving outward from the center, the light appears bluer, perhaps hinting at recent or ongoing star formation within the disk. The edges of the galaxy appear diffuse and less defined, with a faint extension visible, possibly due to tidal interactions or past mergers. There's a slight hint of disturbance in the galaxy's structure, which could indicate minor gravitational interaction with a neighboring galaxy.