The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. The central region exhibits a higher concentration of luminosity, indicative of a substantial galactic nucleus. The galaxy's color profile suggests a population dominated by older stars. There's no readily apparent spiral arm structure or dust lane obscuration. The overall shape is somewhat elongated, with a smooth decline in surface brightness from the center outwards. There are no signs of a major ongoing merger or tidal disturbances, though slight asymmetries in its outer regions could suggest a minor interaction in its past. Based on the color profile and morphology, it's likely a relatively massive galaxy with a quiescent star formation rate.
