The galaxy presents as an elliptical or lenticular type, exhibiting a predominantly smooth morphology with little to no discernible disk-like structure. The central bulge appears prominent and luminous, indicating a high concentration of stars. The galaxy's overall shape is moderately elliptical, not perfectly spherical, but not highly elongated. There is no visible evidence of ongoing major merging activity or strong tidal disturbances. The overall color gradient suggests a population of older stars, with a redder hue in the outer regions compared to the central bulge. Star formation activity appears low or negligible. 
