The galaxy appears as a generally smooth, elliptical-shaped object with a bright, concentrated central bulge. The light distribution suggests a relatively evolved stellar population, with the yellowish-white hue indicating the presence of older, lower-mass stars. There's a subtle elongation visible, hinting at a slightly cigar-shaped morphology. Overall, the galaxy appears to be relatively isolated and undisturbed, without any signs of ongoing major mergers or tidal interactions. The outer regions of the galaxy fade gradually into the background sky, suggesting a fairly smooth transition in stellar density.
