The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal with no discernible spiral arm structure or prominent dust lanes. The color profile suggests a significant population of older stars, indicated by the predominantly yellow-red hue, indicative of lower levels of current star formation activity. The galaxy exhibits a high degree of central concentration, with the intensity of light diminishing gradually towards the outer edges. There is no visually apparent evidence of ongoing merging activity or major tidal disturbances in this image. It displays a fairly round shape, although slightly elongated.
