The galaxy presents as a relatively small, compact object. Its morphology appears largely smooth, lacking significant discernible features such as spiral arms or a prominent disk structure. The light distribution indicates a centrally concentrated brightness profile. The color is noticeably blue, suggesting the presence of a younger stellar population and ongoing star formation activity, particularly concentrated toward the center. Its shape seems generally round. A very slight irregularity or minor perturbation is possibly present in the outer reaches of the galaxy, although it is not very significant. No strong evidence of a major ongoing merger is apparent. 
