The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core region exhibits a bright, concentrated luminosity. Radially outward from the core, the luminosity gradually decreases, displaying a faint, diffuse halo. The color profile suggests a dominant older stellar population, with a slightly redder hue toward the core and subtle bluer regions toward the outer edges. It shows an elliptical shape, although approaching circular with no evident spiral arm structure or strong morphological disturbances. There is no indication of a recent major merger event, although some minor irregularities in the outer halo could suggest interactions with smaller companions in the past.
