The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is bright in the g, r, and z bands, indicating a significant population of older stars. The galaxy appears largely featureless, with a high degree of symmetry. There is no strong evidence of prominent spiral arms or a distinct disk structure. The galaxy's round shape is slightly elongated. There's some subtle evidence of tidal disturbances or potential merger activity. Overall, the object appears to be a massive galaxy, possibly a lenticular or elliptical type, with a considerable stellar mass and relatively low star formation rate.
