The galaxy appears to be an elliptical galaxy, presenting a largely smooth and featureless morphology. The central region exhibits a concentrated luminosity, with a gradual decrease in brightness toward the outer edges. The galaxy appears largely spheroid in shape, displaying a slight elongation. There is no evidence of a prominent disk structure or spiral arms. The color profile indicates a population of older stars. There is no noticeable dust lane or signs of active star formation within the galaxy. There is no evidence of ongoing or recent merger activity or major tidal disturbances.
