The galaxy exhibits a concentrated morphology, appearing largely elliptical in shape with a smooth light distribution. It has a bright central bulge which contributes significantly to its overall luminosity. The radial light profile appears steep, diminishing rapidly from the core outwards. The galaxy is slightly elongated, with a relatively high degree of symmetry. There is no obvious presence of spiral arms or dust lanes. The color gradient suggests a population of older stars, giving it a yellowish hue. Evidence indicates that the galaxy has a very low rate of star formation. The lack of significant irregular features suggests it is not undergoing a major merging event. Based on its smooth appearance, it is likely an early-type galaxy.
