The galaxy presents an elliptical morphology, though some irregularities are apparent, suggesting a possible ongoing interaction. The central region displays a concentrated, bright core, which is redder in color, potentially indicating an older stellar population. Extending outwards from the core, the galaxy exhibits a diffuse halo of light, appearing bluer in hue, suggesting the presence of younger stars.

The overall structure appears somewhat disturbed, with a possible tidal feature extending to one side. This disturbance could be indicative of a minor merger event or close interaction with another galaxy. There is a slight asymmetry in the light distribution, further supporting the hypothesis of a non-equilibrium state.

Given the observed color gradients and morphological features, this galaxy is likely undergoing active star formation, albeit potentially triggered by the aforementioned interaction.
