The galaxy presents a generally smooth, elliptical morphology. The core region exhibits a concentrated, bright luminosity, transitioning to a more diffuse outer halo. There is an indication of a minor extended feature emanating from the main galactic body, possibly a tidal tail or a plume resulting from gravitational interaction. The color profile suggests an older stellar population, with a redder hue dominating the galaxy's light, particularly in the central bulge. Star formation appears subdued, if present, with an absence of prominent blue regions indicative of young, hot stars. Overall, the galaxy appears as a mature, relatively undisturbed system.
