The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge, transitioning outwards to a less dense halo. The color gradient suggests a predominantly older stellar population, with a yellowish hue dominating the core, which may indicate a lack of significant recent star formation. There appears to be some disturbances in the symmetry of the galaxy, such as a very subtle hint of tidal tails and some light warping, possibly caused by gravitational interactions. No prominent spiral arm structures or distinct dust lanes are discernible.
