The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears nearly round. There is a subtle color gradient, transitioning from a slightly bluer hue in the central region to a redder tint toward the outer edges. The light distribution appears quite even, lacking any distinct spiral arms or prominent star-forming regions. There are no significant signs of recent merger activity, although a very minor asymmetry cannot be entirely ruled out. The galaxy appears to be a mature system, with a relatively low current star formation rate.
