The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arm structures or distinct features. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The galaxy has a generally round shape. There is no clear indication of ongoing major mergers, though subtle asymmetry might indicate minor gravitational interaction or internal disturbances. The overall color suggests a redder stellar population, characteristic of galaxies with lower star formation rates. The estimated size implies this is a moderately large galaxy.
