The galaxy appears as a generally smooth object with an elliptical morphology. Its color profile indicates a population of older stars, contributing to the overall redder hue. The concentration of light suggests a prominent central bulge. There may be some evidence of a faint disk component that is difficult to resolve. No spiral arms are visible. The galaxy does not show any obvious signs of interaction with another galaxy or any disturbances in its overall structure. The light distribution is fairly symmetric across the galaxy, lacking any clear knots or regions of intense star formation.
