The galaxy presents as a single, dominant object with a generally smooth morphology. Its shape is elliptical, appearing somewhere between round and cigar-shaped. It presents with a bright, concentrated core that emits light across multiple visible bands; however, it is brightest in the redder bands. There is no obvious disk structure or spiral arm morphology observed. There does not appear to be any evidence of ongoing or recent major merging activity or any significant tidal disturbances. Faint, diffuse light extends outwards from the core, diminishing with distance. This extended light appears to be smoothly distributed. The overall color suggests a population of older stars and a relatively low rate of ongoing star formation.
