The galaxy presents as an elliptical morphology, appearing largely featureless and smooth in its light distribution. Its color profile suggests a more evolved stellar population, with a slightly reddish hue. The galaxy exhibits a concentrated central region, which gradually fades into its outer regions. There is no apparent structure indicating spiral arms or a distinct disk component. There are no visible signs of active galactic nuclei or any significant dust lanes. The shape is closer to "in between" from round or cigar shaped. Furthermore, the galaxy appears isolated.
