This galaxy exhibits a primarily smooth morphology, lacking discernible spiral arms or other distinct features. It appears nearly circular, suggesting a possible classification as an elliptical galaxy. The galaxy presents a relatively concentrated light profile, with the luminosity decreasing gradually from the center outwards. The color is somewhat yellowish-white in the center, indicative of a population of older stars. The overall red color may be due to dust obscuration or the dominance of older stellar populations. There is no evidence of any tidal disturbances or interactions with other galaxies, suggesting it is a relatively isolated system. At a redshift of approximately 0.3, this galaxy is at a significant distance.
