The galaxy presents as a centrally concentrated object, appearing generally smooth in texture, with hints of a flattened, disk-like morphology. The color gradient transitions from a bluer, brighter central region to a redder, fainter outer halo, suggesting a more evolved stellar population in the outer regions. While predominantly smooth, subtle irregularities in the galaxy's structure suggest a possible minor interaction or disturbance event. Overall, this galaxy appears to be of intermediate mass and exhibiting a modest rate of star formation, with no indications of a major ongoing merger event.
