The galaxy presents a generally smooth morphology, appearing largely featureless with a dominant spheroid component. It exhibits a concentrated, rounded central region that gradually diffuses outward, indicative of an elliptical galaxy. There is a possible faint plume or tidal feature extending from the main body of the galaxy.

The color profile suggests a population of older stars, leaning toward the redder end of the spectrum, implying minimal ongoing star formation. The galaxy appears relatively isolated, although there is a galaxy located nearby. There do not seem to be any signs of major disturbances.
