The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is somewhat elliptical, tending toward round. There is a subtle variation in color across the galaxy, hinting at a population gradient, with the central region appearing slightly redder compared to the outer regions. This could indicate an older stellar population in the core. The outer regions exhibit a bluer hue, possibly indicating more recent or ongoing star formation activity, although not dramatically so. There is a hint of subtle features which might indicate interactions with smaller galaxies. Overall, the galaxy appears to be relatively massive, based on its size and luminosity.
