The galaxy presents as a largely featureless elliptical or lenticular structure, exhibiting a smooth, diffuse luminosity profile. Its shape appears moderately rounded, without a significant elongation or asymmetry suggesting a highly disturbed system. The color profile indicates a population of older stars, given the redder hue in the observed bands. There are no immediately apparent spiral arms, bars, or prominent dust lanes. The galaxy shows no signs of a major ongoing merger event, though a minor disturbance cannot be fully ruled out. Its effective radius is relatively small. Given the estimated stellar mass, this object is a moderately massive galaxy with little current star formation activity.
