The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that transitions smoothly into a more diffuse halo. The galaxy's color profile suggests a relatively evolved stellar population, with a dominant yellow hue in the central regions. There is little evidence of spiral arms or significant dust lanes. The overall structure appears undisturbed, indicating no recent major merger events, with a hint of possible minor disturbances. The object possesses a roughly round shape, as opposed to a highly elongated or irregular form. Based on the color, mass, and indications of star formation properties, this galaxy exhibits what seems to be a rate of star formation, with a hint of the potential of a more active past.
