The galaxy appears to be a relatively smooth, elliptical type, exhibiting a centrally concentrated light profile. There are no prominent spiral arms or a distinct disk structure visible, implying a lack of significant ongoing star formation in a flattened structure. The galaxy's shape is generally elongated, but not dramatically so, with an intermediate level of ellipticity. There is a subtle color gradient, with the central region appearing slightly bluer than the outer halo, which exhibits a more reddish hue, potentially indicating a difference in stellar populations between the core and the outskirts. There is no obvious evidence of major mergers or strong tidal features that would suggest a recent, disruptive interaction with another galaxy. Minor disturbances or irregularities cannot be ruled out, but the overall structure appears relatively relaxed and undisturbed. The galaxy's size appears to be moderate, neither exceptionally large nor particularly small.
