The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The core exhibits a concentrated, bright luminosity, suggestive of an older stellar population dominating the central region. Moving outward from the core, the luminosity gradually decreases, with a relatively smooth transition to the outer regions. There are subtle color variations, with the central regions appearing slightly more yellow, transitioning to a bluer hue in the outer regions, possibly indicating some ongoing star formation further from the galactic center, but not significantly. The overall shape is generally round, with no apparent signs of strong tidal disturbances or major mergers, though a slight asymmetry could hint at minor gravitational interactions in its past.
