The galaxy presents a predominantly smooth, elliptical morphology. It appears to be relatively featureless, lacking prominent spiral arms or a distinct disk structure. The galaxy exhibits a centrally concentrated luminosity profile, with a bright, well-defined core that gradually diminishes in intensity towards the outer regions. Color gradients suggest a population of older stars, particularly within the core, with possibly a subtle presence of younger, bluer stars in the surrounding regions. There is little evidence of significant ongoing star formation activity. The overall appearance is consistent with a galaxy that has undergone a period of quiescence. There is a subtle, very minor indication of a possible tidal disturbance to the system, but overall, the galaxy appears relatively undisturbed.
