The galaxy appears as a concentrated, elliptical-shaped structure. It exhibits a smooth, relatively featureless morphology with a high degree of central concentration. The color gradient suggests a dominant older stellar population, with light primarily in the redder bands and diminished light in the blue end of the spectrum. There are no clearly defined spiral arms, bars, or dust lanes visible. There is a slight elongation in its shape, deviating from being perfectly circular, suggesting a possible minor interaction or internal rotation effects. Overall, the galaxy's morphology indicates it is likely an early-type galaxy.
