The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The galaxy's light profile appears highly centrally concentrated, with a gradual decrease in intensity moving outwards from the core. The overall shape approximates a circle and does not present with any strong indications of a disk or spiral arm structure upon initial inspection. The color suggests a population of older stars, indicative of a lower star formation rate. There may be minor irregularities, but these are very subtle and do not obviously indicate a recent major merger event or significant tidal disturbance.
