The galaxy presents as a relatively smooth, elliptical-like structure. There is a bright, concentrated central bulge exhibiting a yellowish hue, possibly indicative of an older stellar population. Fainter, bluish regions extend outwards, forming a diffuse disk. These regions may indicate areas of more recent, ongoing star formation, contrasting with the dominant older population in the bulge. The galaxy's shape is somewhat elongated, but not distinctly cigar-shaped. There are no obvious signs of major mergers or significant tidal disturbances, although subtle asymmetries and irregularities within the outer disk could suggest minor gravitational interactions. The overall structure suggests a galaxy that is transitioning from a more actively star-forming state towards a quiescent, elliptical morphology.
