The galaxy exhibits a smooth, concentrated morphology, appearing largely featureless without prominent spiral arms or a distinct bar structure. Its overall shape is elliptical, with a slight flattening. The core is bright and concentrated, indicating a high density of stars. There is a gradual decrease in luminosity moving outward from the core. The galaxy's color is slightly redder, suggesting an older stellar population and a relatively low rate of ongoing star formation. There is no apparent dust lane or clear evidence of a recent major merger event.
