The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated light distribution. Its shape is approximately round, showing no signs of strong elongation or a defined disk structure. The light profile suggests a centrally dominant core. The color indices hint at an evolved stellar population, dominated by older stars that emit strongly in the redder wavelengths. No clear spiral arms or prominent star-forming regions are discernible within the galaxy's morphology, which points to a lack of significant ongoing star formation. There is no apparent interaction with nearby galaxies, and the object presents a largely undisturbed morphology. The lack of any visible disturbances in the overall structure suggests that it is not undergoing any major merging events.
