The galaxy presents as a largely smooth, elliptical-like structure. Its core exhibits a concentrated, bright glow, suggesting a high density of stars and/or an active galactic nucleus. Moving outward from the core, the light intensity diminishes gradually, indicating a decreasing stellar density with radius. There is a slight elongation noticeable, although the object is mostly spheroidal. The galaxy's color appears yellowish-orange, which could indicate an older stellar population dominated by redder stars. No prominent spiral arms or dust lanes are evident, reinforcing the impression of a relatively undisturbed, evolved system. There are no signs of major mergers or significant tidal disturbances, but a possible minor disturbance cannot be ruled out. The overall morphology points towards an early-type galaxy with a substantial stellar mass and relatively low star formation activity.
