The galaxy appears as a slightly elongated, elliptical-like structure. It exhibits a smooth, featureless morphology with a concentrated central bulge that dominates the overall light distribution. The light appears to gradually fade outwards from the core, with no discernible spiral arms or prominent dust lanes visible. A very slight hint of bluer color is observed around the outskirts of the galaxy, hinting at some low level star formation. There are no signs of active galactic nuclei or major mergers, although it is possible that there is a minor disturbance affecting its overall structure. The estimated half-light radius suggests that it is an intermediate sized galaxy. Its dominant color appears to be reddish/yellow, implying that older stellar populations comprise the bulk of its observed luminosity.
