The galaxy presents as a relatively smooth, elliptical-like structure. Its core region exhibits a bright, concentrated luminosity, appearing predominantly yellow. The galaxy's light gradually diminishes outward, lacking any sharply defined spiral arms or prominent dust lanes. A slight elongation suggests it may not be perfectly spherical. The overall color indicates a population dominated by older stars, with little evidence of ongoing, intense star formation. There appears to be no substantial morphological disturbance or signs of a major merger event.
