The galaxy presents as a singular, relatively smooth object. Its morphology appears elliptical, although a slight deviation from perfect roundness suggests it may be more accurately described as an intermediate elliptical form. The color profile exhibits a dominant yellowish-orange hue concentrated towards the galactic center, likely indicating a population of older stars. Fainter blue tinges are present along one edge of the galaxy. These regions may signify areas of more recent, albeit subdued, star formation. There is no immediately apparent spiral structure or bar feature. No evidence of ongoing major mergers or tidal disruption is observed, though a slight asymmetry on its top left might suggest a past minor interaction or internal perturbation.
