The galaxy presents as a generally smooth, elliptical structure with a prominent central bulge. It exhibits a moderately bright, diffuse glow, suggesting a population of evolved stars. There's a slight elongation in its shape, with a ratio indicating a moderate deviation from perfect circularity. The absence of clear spiral arms or dust lanes points towards a classification as an early-type galaxy. A subtle color gradient is observed, where the central region appears slightly bluer than the outer regions. The galaxy does not appear to be undergoing any major mergers or tidal disturbances. Overall, the morphology suggests a relatively relaxed and stable system.
