The galaxy appears as a single, relatively smooth object with a generally elliptical morphology. A lack of distinct spiral arm structures is observed. The core exhibits high luminosity, appearing nearly white. There is a radial color gradient, transitioning from a yellowish-white core to more orange hues in the outer regions. The galaxy shows moderate apparent roundness, lacking strong elongation. There are suggestions of tidal disturbances, perhaps minor, and there is a distinct possibility that the galaxy is undergoing a merger. Overall, the object appears to be a relatively massive galaxy, possibly an elliptical galaxy with characteristics indicating ongoing or recent interaction. The low star formation rate is also a factor to consider when determining what type of galaxy it is.
