The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color profile suggests a dominant population of older stars, particularly within the central region, exhibiting a yellowish-orange hue. The outer regions show a gradual fading in intensity. There is little evidence of spiral arm structure or significant dust lanes. The overall morphology suggests a lack of recent major merger events or intense star formation activity. The shape appears to be slightly elongated. While there may be some minor disturbances, the general structure seems undisturbed.
