The galaxy exhibits a primarily elliptical morphology with a notable central bulge. The bulge appears bright and concentrated, suggesting a significant population of older stars. A diffuse halo surrounds the central bulge, exhibiting a slightly flattened shape. Faint spiral arm structures are suspected within the halo, though not sharply defined. Overall color is indicative of a mix of stellar populations, with the bulge leaning towards warmer (redder) colors, and the outer regions showing bluer hues, possibly due to the presence of younger stars and ongoing star formation. There is some evidence of disturbance in the outer disk. There is no definitive presence of a stellar bar.
