The galaxy presents an overall smooth morphology with a hint of a disk-like structure. The central bulge appears bright and yellowish, suggesting an older stellar population with less active star formation in this region. The galaxy exhibits an elongated, cigar-shaped appearance. There is no obvious evidence of significant ongoing mergers or major disturbances in the galaxy's structure, although some minor irregularities or faint features cannot be ruled out with the available image resolution. The overall color suggests that star formation is more subdued, particularly within the bulge, however the bluer edges indicate ongoing star formation.
