The galaxy presents as a relatively smooth, elliptical morphology. Its central region exhibits a concentrated, bright core, suggestive of a high stellar density. The color gradient transitions from a yellowish-white at the core to a slightly redder hue in the outer regions. The overall shape is elongated, displaying a notable deviation from perfect circularity. There appears to be a subtle warping or disturbance in the morphology, hinting at possible gravitational interactions or past merger events. The galaxy's extent indicates a substantial size, with a considerable radius. The relatively uniform color distribution suggests a passively evolving stellar population, likely dominated by older, redder stars, and a low ongoing star formation rate.
