The galaxy presents an elliptical morphology, appearing as a flattened spheroid in this projection. A smooth light distribution is observed, with a concentration of luminosity towards the center of the galaxy. There is a discernible color gradient; the core exhibits a yellowish-orange hue, transitioning to a bluer tint in the outer regions. This color variation may imply differences in stellar populations or dust content across the galaxy's radial profile. The lack of distinct spiral arms or prominent dust lanes suggests that the galaxy is most likely an early-type system. Minor asymmetries or subtle irregularities in the outer regions cannot be entirely discounted, pending higher-resolution imaging and spectral analysis.
