The galaxy presents as an elliptical morphology with a high degree of central concentration, indicating a significant bulge component. The light distribution transitions smoothly from the bright, yellowish core to the fainter, bluish outer regions. The color gradient suggests the presence of older stellar populations in the central region, with a possible increase in younger, bluer stars in the outer disk. The isophotes appear to be mostly smooth and symmetric with the exception of the the top of the image, suggesting no ongoing major mergers. The slight ellipticity indicates some level of rotational support. The galaxy appears relatively isolated, without any signs of tidal interactions or close companions within the immediate field. The overall structure is consistent with a galaxy that has undergone significant evolutionary processing and is relatively quiescent in terms of star formation.
