The galaxy presents a centrally concentrated morphology, with a bright, yellowish core region that gradually diffuses outwards. The overall shape appears elliptical, transitioning from a brighter, more defined center to a fainter, less structured halo. There is evidence of blueish-tinted regions within the galaxy's body which may indicate areas of recent or ongoing star formation. The outer regions lack distinct spiral arm structures or other clear features, appearing relatively smooth and unstructured. There are no signs of major ongoing mergers or tidal disturbances, though some minor irregularities cannot be ruled out. The galaxy appears to be somewhat isolated, with no nearby interacting galaxies evident in the immediate field of view. The size of the object is small, but the flux is high, leading to the possibility that this is a relatively massive galaxy.
