The galaxy presents as a relatively compact object with a bright, concentrated core. The overall shape is somewhat elliptical, but with subtle irregularities suggesting possible disturbances or tidal interactions. The central region exhibits a vibrant, almost overexposed, blue-white hue, indicative of a high concentration of hot, young stars or an active galactic nucleus. Fainter, extended emission surrounds the core, fading into the background. This outer region displays a more reddish tint, suggesting an older stellar population. There are hints of asymmetry in the distribution of light within the outer regions, possibly indicating past or ongoing minor merger activity. No prominent spiral arms or bar structures are discernible in the image.
