This galaxy presents a generally smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The light distribution appears centrally concentrated with a gradual decline in intensity outward. The galaxy's shape seems somewhat elliptical, displaying an intermediate degree of roundness. There is no indication of ongoing major mergers or significant tidal disturbances. The galaxy emits light across the g, r, and z bands, with the z-band emission slightly more pronounced. The overall color suggests a potentially older stellar population with relatively low current star formation activity. The estimated size indicates a moderately compact system.