The galaxy presents as a fairly smooth, elliptical object with a high degree of central concentration. The light is dominated by a bright, unresolved core region. The overall shape is close to round with a slight elongation along the horizontal axis. There is little evidence of spiral arm structure or prominent dust lanes. A minor disturbance is suggested by a slight asymmetry in the outer regions. The color profile exhibits a subtle gradient, transitioning from bluer hues in the outer regions to redder hues toward the central bulge, which may indicate older stellar populations are dominant in the center. The galaxy appears to be relatively isolated, showing no clear signs of a major ongoing merger, though some tidal features cannot be ruled out. Based on its morphology, this galaxy can likely be classified as an early-type galaxy.
