The galaxy presents a generally smooth appearance, suggesting an elliptical morphology. Its light distribution is concentrated towards the center, with a bright, yellowish core indicating a substantial population of older stars. The galaxy's overall shape is close to round, with only a slight deviation from perfect circularity. Fainter, bluer light is observed in the outer regions, possibly indicative of younger stellar populations or ongoing star formation, though its relative amount appears to be lower than that of the core. There are no obvious signs of major disturbances or tidal features, pointing to a relatively isolated evolution. No distinct spiral arms or a well-defined disk structure are apparent.