The galaxy presents a largely smooth, elliptical morphology. It appears moderately concentrated, with a gradual decrease in luminosity from the core to the outer regions. The galaxy's color profile indicates a redder population, indicative of older stars and a relatively quiescent star formation rate. There is a faint hint of a disk-like structure, but it is not well-defined. No significant tidal features, such as tails or bridges, are visible, suggesting it is not currently undergoing a major merger event. The galaxy shows signs of minor disturbances, but is mostly undisturbed. The overall shape appears somewhat in between being round and elliptical.
