The galaxy presents as a diffuse, elongated object with a moderately smooth appearance. It exhibits a subtle color gradient, shifting from a bluer hue at the center to slightly redder tones towards the edges. The overall morphology suggests an elliptical shape, though it deviates somewhat from a perfect ellipse, possibly indicating a mild tidal disturbance or interaction. There is no clearly defined spiral arm structure visible, and the light distribution appears relatively uniform, lacking strong concentrations or knots. The absence of strong, localized emission regions indicates a relatively low star formation rate. The galaxy is inclined to our line of sight, appearing cigar-shaped. Evident signs of interaction or a recent major merger are present. Patches or streams of material are not obvious at this resolution.
