The galaxy exhibits an elongated, cigar-shaped morphology. The central region displays a concentrated, reddish-orange hue, suggesting a relatively older stellar population or significant dust obscuration. Moving outwards from the center, the color transitions to a slightly bluer shade, possibly indicating the presence of younger, hotter stars in the galactic disk. The disk structure appears somewhat disrupted, with hints of faint, irregular features that could be indicative of tidal interactions or minor disturbances. Overall, the galaxy's structure appears relatively smooth, with no readily discernible spiral arms or prominent star-forming regions. The galaxy's red color suggests that the galaxy is passively evolving, or is dust-obscured.