The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge exhibits a pronounced yellowish-orange hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a more greenish tint, with faint blue hints, possibly indicative of some younger stars. The galaxy appears somewhat lenticular in shape, exhibiting a flattened disk-like structure, but lacking distinct spiral arms. Overall, the galaxy appears undisturbed, showing no obvious signs of ongoing or recent major mergers. It is of considerable size, estimated to be approximately 10 kpc across. It is moderately distant, with an observed redshift placing it at a cosmological distance. The star formation activity appears to be low, with older stars and little gas and dust.