The galaxy presents as a somewhat diffuse object, exhibiting an overall elliptical morphology with a relatively smooth light distribution. The color gradient suggests a potential mix of stellar populations, possibly indicating some ongoing or recent star formation activity in the bluer regions. The light appears to be concentrated towards the center, typical of elliptical galaxies, though there are indications of slight disturbances or asymmetries in the outer regions, which could be indicative of minor interactions or past mergers. The dominant color is redder, suggesting a population of older stars is present. The galaxy appears to be relatively isolated within its immediate surroundings. The size of the object suggests it is likely to be a massive galaxy, however, there appears to be no active galactic nuclei.
