The galaxy presents an elliptical morphology, appearing largely smooth and featureless in the observed color bands. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. The overall color profile indicates a primarily older stellar population, contributing to the galaxy's redder hue, with a hint of bluer light toward the outer edges. There is little evidence of significant dust lanes or active star formation regions. Slight asymmetry may indicate a minor tidal disturbance or a recent, small merger event. The isophotes are relatively smooth and concentric. The galaxy displays a moderate inclination relative to the line of sight, providing a slightly elongated appearance. The overall structure appears relatively undisturbed and relaxed.
