The galaxy presents a generally smooth morphology, appearing elliptical in shape, with a high degree of central concentration. It exhibits a notable elongation, suggesting a possible classification towards the S0 or lenticular type, or potentially an elliptical galaxy with significant angular momentum. The color profile indicates an older stellar population, dominant in the redder wavelengths, with some indication of bluer light emission towards the core. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger activity. However, minor irregularities in the outer halo cannot be ruled out at this resolution.
