The galaxy appears as a moderately bright, elliptical-like structure. Its overall shape is somewhat elongated, but not highly flattened. The galaxy's central region exhibits a concentrated luminosity. The galaxy appears to have a smooth, diffuse morphology; there is little or no apparent structure, such as spiral arms or dust lanes. The light distribution smoothly fades from the center outwards. The galaxy's color profile suggests an older stellar population; the galaxy presents a yellow-red hue. There is no apparent evidence of active star formation within the galaxy. Based on the morphology, the galaxy likely contains primarily older stars and has a low specific star formation rate. There appears to be no significant tidal disturbance or any nearby companions.
