The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, appearing almost spherical in shape with a yellowish hue. Moving outward from the core, the light gradually diffuses into the surrounding halo, maintaining a smooth gradient without prominent spiral arm structures or significant dust lane obstruction. The galaxy appears relatively isolated, showing no strong visual evidence of recent or ongoing major merger events, although subtle irregularities could suggest minor gravitational interactions. The overall color profile suggests a stellar population dominated by older, redder stars, characteristic of a more evolved system with suppressed star formation activity. The observed smooth morphology and color suggest the galaxy is an early-type galaxy.
