The galaxy exhibits a predominantly smooth morphology, with minimal discernible features such as spiral arms or a distinct disk structure. The light distribution appears centrally concentrated, characterized by a bright, relatively symmetrical bulge. There is a slight ellipticity, but it is largely rounded in appearance. Color gradients across the galaxy are subtle, with the central region exhibiting a slightly bluer hue compared to the outer regions, which appear redder. This color variation could indicate younger stellar populations in the core and older populations in the halo. There is no prominent dust lane or evidence of ongoing major mergers or significant tidal disturbances, although a subtle asymmetry might suggest minor past interactions. The galaxy presents a relatively evolved system, likely a lenticular or early-type spiral galaxy transitioning towards a more quiescent state.
