The galaxy presents as a somewhat elliptical structure with a bright, concentrated central region. A fainter, more diffuse halo extends outwards. The main body of the galaxy exhibits a relatively smooth texture, lacking clearly defined spiral arms or prominent dust lanes in the visible spectrum. The overall color gradient suggests a population of older stars dominating the central bulge, with potentially a younger, bluer stellar population contributing to the light in the outer regions, although this is not distinctly apparent. There is an indication of slight disturbances to the morphological structure. Overall, the galaxy appears to be an intermediate-sized system that could potentially be an elliptical or lenticular galaxy.
