The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. Its color appears to be predominantly yellow-orange, suggesting a population of older stars. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape, and the lack of discernable spiral arms or dust lanes supports its classification as an elliptical galaxy. There is no apparent major disturbance or merging activity, though a minor tidal interaction cannot be completely ruled out based on the slight asymmetry in the outer regions. Given its color and smooth morphology, it is likely a massive galaxy with relatively low ongoing star formation. The estimated half-light radius suggests it is moderately sized.
