The galaxy presents a primarily smooth morphology, with an elliptical appearance. The central region exhibits a high degree of luminosity, indicating a concentrated stellar population, likely an older population that has undergone little star formation. The galaxy's overall color profile suggests a redder hue. The lack of prominent spiral arms or dust lanes suggests a classification towards the early-type end of the Hubble sequence. There may be some minor disturbance in the morphology, but the image primarily shows a galaxy that is undisturbed. The galaxy exhibits an intermediate roundness.
