The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge region is characterized by a concentrated, yellow-orange hue, indicative of an older stellar population. The galaxy exhibits a moderate degree of roundness, with a subtle deviation from a perfect circular form, lacking any clear bar structure. There is no visible evidence of a strong disk component, spiral arms, or significant dust lanes. The galaxy's outer regions fade gradually, suggesting a diffuse stellar halo. We do not observe any tidal tails or strong morphological distortions indicating recent major merger activity, though it cannot be ruled out that there could be subtle signs of possible minor disturbance.
