The galaxy presents as an elliptical morphology with a high degree of central concentration. It appears largely smooth in texture with minimal substructure visible within its isophotes. The color index suggests a population of older stars, with a redder hue dominating the galactic light. There is no visual evidence of spiral arms or a prominent disk structure. The galaxy exhibits a well-defined, round shape, indicating a relaxed dynamical state. There is no indication of any recent major merger events, and the overall morphology indicates a quiescent system with little ongoing star formation. The object is small, however, still bright and has very strong definition against the background sky.
