This galaxy presents a somewhat amorphous structure, exhibiting features that suggest both smoothness and some degree of irregularity. It appears to have a central bulge or core that is brighter and more concentrated. Extending outwards from this core, there is evidence of a faint disk-like component, however it is not well-defined. The disk shows hints of subtle disturbances, possibly due to minor gravitational interactions or internal processes.

The color profile of the galaxy indicates a generally bluish hue, potentially signifying the presence of younger stellar populations, though the overall star formation rate is likely low. There is no clear sign of significant dust lanes or spiral arm structures visible in this image. The overall morphology appears to be somewhere between that of an elliptical and a spiral galaxy, potentially representing a transitional or peculiar type.
