The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology. There is a dominance of light towards the core, which could indicate a supermassive black hole and/or a bulge component. It seems that the galaxy may be an elliptical or a lenticular galaxy, as it lacks prominent spiral arm features, but the disk cannot be ruled out with current data. There is some indication that the galaxy is undergoing a merger, or experiencing tidal disturbances. There is a slight asymmetry, indicating a possible interaction or recent merger event. This asymmetry manifests in the irregular distribution of light. The color is biased towards the redder bands. There are some hints of bluer regions in the galaxy, but in general, it appears to be comprised of older stellar populations.
