The galaxy appears to be an elliptical or lenticular galaxy given its generally smooth morphology and lack of discernible spiral arm structure. The light profile suggests a concentrated nucleus that gradually fades toward the edges of the galaxy. The color indices indicate a population of older stars, potentially with relatively low ongoing star formation, contributing to a redder overall hue. The galaxy shows a high degree of symmetry, with minimal signs of tidal disturbances or ongoing major mergers. There are no prominent dust lanes or other features indicating significant amounts of cold gas. The overall round shape of the galaxy points towards a relatively low angular momentum.
