The galaxy presents as a roughly elliptical, concentrated light source. The core exhibits a smooth, centrally condensed profile with a yellow-orange hue, indicative of a stellar population dominated by older, redder stars. There is a slight decrease in surface brightness moving outwards from the core towards the galaxy's periphery, which suggests the light production is not equally distributed. There are no apparent spiral arms or distinct features that would otherwise suggest active star formation or a recent merger event. Its shape indicates a spheroidal morphology, potentially an elliptical galaxy, and lacks significant structural irregularities.
