The galaxy presents an overall smooth morphology, appearing as a relatively rounded object. There is evidence of a central, bright bulge-like structure, with the light appearing more yellow at the very core, possibly indicating an older stellar population. Surrounding this central region, there is a more diffuse, blueish halo of light, potentially representing a younger stellar population or ongoing star formation, albeit at a low rate.  There are some slight irregularities in the outer regions of this halo, but the galaxy does not appear to be significantly disturbed. There is no visible evidence of a prominent disk or spiral structure.  Based on the overall form and color distribution, this galaxy is likely an elliptical or lenticular type.
