The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The light distribution appears centrally symmetric, with no evidence of strong spiral arms or a prominent disk structure. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the galaxy transitions to a bluer colour, potentially indicating a more recent episode of star formation in the outer regions. The galaxy's overall shape deviates somewhat from perfect sphericity, appearing more elongated or cigar shaped. There is subtle evidence of minor asymmetry or disturbances in its outer regions but nothing suggesting any ongoing major merger events. Overall, this galaxy presents characteristics consistent with a relatively massive system with ongoing but low-level star formation.
