The galaxy appears as a slightly elongated, smooth object with a concentrated central region. The light distribution suggests an elliptical morphology with little to no evidence of spiral arms or a disk structure. The galaxy exhibits a yellowish-orange color, which could indicate an older stellar population with lower levels of ongoing star formation. The morphology appears undisturbed, lacking significant tidal features or distortions suggestive of recent major mergers, though minor disturbances cannot be ruled out. The object's overall roundness indicates a relatively relaxed dynamical state.
