The galaxy presents as an elliptical morphology, elongated in shape with a notable lack of distinct spiral arm structures or prominent dust lanes. Its color profile indicates a concentration of older stellar populations, suggested by the yellowish-white hue that dominates its central region, likely indicating a cessation, or at least a reduction, in star formation activity. The smooth, almost featureless appearance, supports a classification as an early-type galaxy where a spheroidal component contributes a larger portion of the luminosity. The outer regions display a faint blue tinge indicating the presence of small, young stars. There appears to be no significant morphological disturbance or ongoing major merger activity visible, giving the impression of a relatively settled system. Overall, the galaxy is likely a mature, quiescent system, nearing a state where star formation is minimal or absent, with the blue tinge suggesting possible rejuvenation.
