The galaxy presents as an elliptical morphology, characterized by a smooth, centrally concentrated light distribution. Its overall shape is somewhat elongated, appearing to be in between a round and cigar-shaped configuration. There is little to no evidence of spiral arm structure or significant dust lanes. The color profile suggests a relatively older stellar population, with a dominant yellowish hue emanating from the galactic center. There appears to be little to no evidence of active star formation within the galaxy. No signs of a recent or ongoing merger with another galaxy are observed. Minor asymmetry may be present.
