The galaxy presents as a relatively smooth, centrally concentrated object. Its shape appears largely elliptical, with a high degree of roundness. There are no prominent spiral arms or bar structures visible, nor significant dust lanes that are immediately obvious. The galaxy exhibits a notable color gradient, appearing more yellow/orange in the central region, indicating an older stellar population. Moving outwards, the color shifts slightly towards red, suggesting a mix of stellar populations. There is no visually significant evidence of ongoing major merging events or tidal disturbances, although there may be slight irregularities that hint at minor gravitational interactions. Overall, the galaxy seems to be a fairly well-formed, evolved system with characteristics of an elliptical galaxy.
