The galaxy appears as a yellowish-white, somewhat diffuse object. It exhibits a largely smooth morphology, with no apparent spiral arms or prominent disk structure visible in this image. The overall shape approximates a circular or elliptical form, displaying a high degree of radial symmetry. There are no significant signs of ongoing mergers or major tidal disturbances discernible within the frame, though subtle internal features cannot be ruled out without higher resolution imaging. The galaxy demonstrates a notable luminosity, suggesting a substantial stellar population and/or active galactic nucleus, and is likely of significant mass. Based on its color profile, the stellar population likely consists of older, redder stars.
