The galaxy presents as an elliptical morphology, with a high degree of visual smoothness, showing no discernible spiral arm structures or prominent dust lanes. Its shape appears to be somewhat elongated, deviating from a perfect circle, with an axis ratio suggesting it might be classified as an E4 or E5 galaxy on the Hubble sequence. The core region exhibits a concentrated luminosity profile, appearing significantly brighter and more yellow than the outer regions. The color gradient shifts from the yellower core to slightly bluer hues in the outer regions of the galaxy, which could indicate some ongoing star formation. There appear to be no signs of a major merger or significant tidal disturbances. The general form of the galaxy suggests it is a relatively undisturbed system with moderate star formation activity for its type.
