The galaxy appears to be a relatively smooth, centrally concentrated system. There is evidence of a disk structure, though it is not highly prominent. The central bulge appears yellowish-orange, suggesting an older stellar population and relatively low levels of ongoing star formation. Extending outwards from the center, there appears to be a fainter, bluish component, indicating the presence of a younger, bluer stellar population, albeit at a lower density. There is marginal evidence of a minor disturbance, likely due to a possible past interaction with a satellite galaxy. Overall, this galaxy appears to be in a transitional phase, possibly evolving from a spiral to a more lenticular or elliptical morphology.
