The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy with a centrally concentrated bulge. There is a slight elongation, indicating it is not perfectly spherical. The central region is bright and yellowish-white, suggesting an older stellar population with fewer young, massive stars. Some bluer light is observed to the right side of the galaxy, which may point to a region of star formation, albeit low. The outer regions are fainter and blend smoothly into the background sky. There is no evidence of strong spiral arms or significant dust lanes. The overall structure suggests a gravitationally relaxed system with a moderate mass and low star formation activity. There might be a minor interaction or disturbance within the galaxy's structure.
