The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. Its color profile suggests a population of older stars, exhibiting a yellowish-red hue, implying reduced star formation activity. The overall shape appears moderately elliptical, with a subtle elongation along one axis. There is no obvious presence of spiral arms or a prominent disk structure, and no evidence of major tidal disturbances. Faint traces of asymmetry or minor disturbances can be observed within the galaxy's structure.
