The galaxy appears as a moderately luminous, elliptical system. It exhibits a generally smooth morphology, with a high degree of central concentration. There is no obvious disk structure or spiral arm features visible. The color profile suggests a population of older stars, indicated by the redder hue. There is no clear sign of active star formation in this system. The galaxy is relatively isolated. It is classified as a single system showing no signs of disturbance or merging activity.
