The galaxy presents as an elliptical type, exhibiting a generally smooth and concentrated morphology. The light distribution appears centrally concentrated with a noticeable radial falloff in surface brightness. The object's overall shape is moderately elliptical, deviating somewhat from a perfectly circular form. Evidence of a disk structure or spiral arms is absent. Subtle color variations are present, with the core exhibiting a slightly yellower hue compared to the outer regions, potentially indicating an older stellar population centrally located. There is no apparent indication of significant ongoing star formation activity based on the available data. Close inspection reveals no signs of major mergers or tidal disturbances, though the possibility of minor interactions with nearby objects cannot be entirely ruled out based on this image alone.
