The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that dominates the overall light profile. The color suggests an older stellar population within the bulge, appearing yellower. Extending outward from the core is a fainter, more diffuse halo of light, showing a gradual decline in surface brightness. A slight elongation is noticeable, suggesting a departure from perfect circularity, more leaning towards an oblate spheroid. There are no prominent spiral arms or significant dust lanes visible, and the overall structure appears undisturbed, indicating the absence of any recent major merger events or interactions.
