The galaxy presents as a relatively smooth, elliptical structure. Its morphology appears largely featureless, lacking prominent spiral arms or a distinct bar. The core region exhibits a higher concentration of luminosity, indicating a central bulge that may be composed of older stellar populations, implied by the color. The galaxy's overall shape appears moderately elliptical, deviating only slightly from a circular form. There is some evidence of disturbance, possibly indicating a minor interaction or past merger event, however this is not conclusive. Overall, the light distribution suggests a mature, potentially quiescent galaxy with relatively low levels of current star formation. The galaxy is a relatively luminous object at its given distance.
