The galaxy presents as a relatively smooth, centrally concentrated object. There is a bright central bulge, which dominates the light profile. Surrounding the bulge, there is a fainter, more diffuse disk. The disk appears to be slightly elongated, deviating from a perfectly circular shape. There is no strong evidence of spiral arm structure. The galaxy displays a color gradient, with the central bulge appearing more yellow, and the outer disk showing hints of blue, which could indicate the presence of younger stars and ongoing star formation in the disk. The overall appearance suggests a galaxy that is somewhere between an elliptical and a spiral, possibly a lenticular type. There are some hints of disturbances possibly indicating a past interaction, but further investigation will be needed.
