The galaxy presents a generally smooth and rounded morphology. There is a subtle colour gradient, the central region appears more yellow/orange-shifted, suggesting an older stellar population and reduced star formation activity in this area. The outer regions show a hint of bluer colour, potentially indicating the presence of younger, hotter stars, albeit at a low rate. There is a subtle indication of very weak spiral arm features, though this is not definitive. The galaxy does not show strong evidence of recent or ongoing major merging activity or significant tidal disturbances. It appears to be a relatively undisturbed system, possibly an early-type spiral galaxy or a lenticular galaxy, with a significant bulge component.
