The galaxy presents an elliptical morphology, characterized by a smooth, diffuse light distribution. Its shape is elongated, with an apparent flattening. The central region exhibits higher luminosity, suggesting a concentration of stars towards the core, possibly indicating an older stellar population. A subtle color gradient is observed, trending towards slightly redder hues in the central region. No distinct spiral arm structures or prominent dust lanes are apparent, supporting its classification as an elliptical galaxy. The lack of defined features indicates a relatively evolved system, potentially nearing the end of its star formation activity. A smaller, fainter object is observed in close proximity, possibly gravitationally interacting or simply a line-of-sight coincidence.
