The galaxy presents as a relatively smooth, elliptical-like structure. The color gradient transitions from a yellowish-white core to a redder outer halo. The central region exhibits a concentrated luminosity, indicating a likely dense population of stars. While no distinct spiral arms are visible, there is a slight elongation to the structure. There are no visible signs of active merging or tidal disruption, though subtle disturbances cannot be ruled out at this resolution. The overall morphology suggests an evolved system, possibly with a relatively low star formation rate. The light profile appears to follow a de Vaucouleurs profile, consistent with an elliptical galaxy classification.
