The galaxy presents as a relatively compact object, displaying a predominantly smooth morphology with a slight elongation. A subtle hint of a disk-like structure is possibly discernible. The galaxy exhibits a color gradient, appearing bluer towards the outer regions and redder towards the core. There is no strong evidence of active galactic nuclei activity or signs of recent major mergers or significant tidal disturbances. The overall impression is of a galaxy with intermediate characteristics between elliptical and spiral types.
