The galaxy presents as a relatively compact object with a central, bright core region. This central region exhibits a bluish hue, possibly indicative of active star formation or an active galactic nucleus. Surrounding the core, a fainter, diffuse structure can be observed. This outer region appears to be relatively smooth with some subtle irregularities or possibly faint arm-like structures. There is an apparent faint hint of a possible merging event. The overall morphology appears to be trending towards a smoother, less defined structure. Further analysis is needed to confirm the nature of the core and confirm any irregularities in its structure.
