The galaxy appears to be a relatively compact elliptical. It exhibits a smooth, concentrated light profile, with the highest luminosity concentrated towards the central region. There is a noticeable radial decrease in surface brightness moving outwards from the core. The galaxy displays a generally round morphology, showing minimal evidence of a disk-like structure or significant tidal disturbances. There are hints of a slightly extended halo around the core of the galaxy. The object's color suggests an older stellar population, with a redder overall appearance. There is a low likelihood of on-going major merging activity or significant star formation. Any star formation is likely suppressed.
