The galaxy presents as a centrally concentrated object, with a predominantly smooth morphology. There is little evidence of spiral arm structure or distinct features typically associated with disk galaxies. The light distribution appears spheroidal, with a noticeable radial gradient in brightness, peaking at the galactic center.

The color profile suggests a population of older stars, indicated by the redder hues concentrated towards the core. Fainter blue light on the outskirts may indicate some younger stellar populations, or star formation occuring at a low rate. There are no indications of ongoing major merging events or significant tidal disturbances. The object appears relatively undisturbed and well-defined within its surrounding environment. 
