The galaxy presents as a relatively smooth, centralized structure. There is a clear, bright core, possibly indicating an active galactic nucleus or a dense concentration of stars. The overall morphology appears elliptical or lenticular, with a gradual decrease in luminosity moving outwards from the core. No distinct spiral arms or bar features are discernible within the limitations of the image resolution. The colour profile seems slightly bluer in the central regions, potentially suggesting ongoing star formation, although the rate is likely not exceedingly high. No strong signs of tidal disturbances or major merger events are apparent. There is some indication of minor asymmetry or subtle features within the galaxy's extended halo, which could denote minor interactions or past accretions.
