The galaxy presents a generally smooth, elliptical morphology. Its color profile exhibits a dominant yellow-orange hue, suggesting a population of older stars and a relatively low rate of ongoing star formation. The galaxy's shape appears elongated, with a ratio of approximately 5:1 along its major and minor axes. There is no visible evidence of spiral arms or a distinct disk structure. The surface brightness distribution appears concentrated toward the central region, with a gradual decrease in brightness outwards. No tidal features or signs of recent major merger events are discernible. There is an overall lack of blue coloration indicating it is likely a more evolved system.