The galaxy presents as a largely smooth, rounded object. It exhibits a concentrated central region, indicating a substantial bulge component. The color profile suggests an older stellar population, with a yellowish-red hue dominant throughout the galaxy's structure. There is little evidence of active star formation, based on the lack of prominent blue or irregular features. The overall morphology suggests a relatively evolved system, consistent with an elliptical or S0 galaxy classification. Minor asymmetry is observed in the isophotes, which could suggest a weak interaction or disturbance, but the overall structure is fairly relaxed and symmetric. The galaxy lacks any obvious spiral arm structures or dust lanes.
