This galaxy exhibits an elongated, cigar-shaped morphology. The central region appears bright and smooth, with a yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the color shifts slightly towards a redder tone, indicating the presence of dust or potentially a change in stellar population age. The galaxy lacks distinct spiral arm structures, and there is no strong evidence of active star formation regions visible in this image. There appears to be little to no disturbance of the galaxy, suggesting it is not undergoing any recent merging activity. The outer edges are indistinct, and the smooth morphology of the core dominates the overall structure.
