The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. It displays a concentrated central bulge that emits light across the g, r, and z bands. There is a slight elongation of the light distribution, deviating from a perfectly circular shape, but it is mostly round in appearance. There is no evident sign of spiral arms or a well-defined disk structure. Color gradients suggest that older stellar populations dominate its composition, with minimal evidence of ongoing major star formation. Based on the shape and lack of obvious features, there is no ongoing merging or tidal interactions with other galaxies. It seems to be an isolated system, consistent with a relatively undisturbed evolutionary history.