This galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central bulge that presents a slightly reddish hue, possibly indicating an older stellar population within the core. The outer regions are more diffuse, appearing fainter and bluer, suggesting the presence of a younger, star-forming population in the extended disk. While a clear spiral structure is not evident, subtle irregularities hint at possible minor disturbances, potentially due to past interactions or minor mergers. The overall shape is somewhat elongated, leaning towards a slightly cigar-shaped morphology. No prominent tidal tails or strong signs of ongoing major mergers are visible.
