The galaxy presents as a generally smooth object with a slight elongation. It exhibits a bright central region, possibly indicative of a significant concentration of older stars or an active galactic nucleus. The color profile suggests a population of stars that are more characteristic of older stellar populations, with a weak emission in blue wavelength bands. The galaxy's morphology appears relatively undisturbed, showing no strong signs of ongoing major mergers or tidal interactions. The object seems to be transitioning between elliptical and lenticular type, showing no distinctive disk and spiral arm structures. Overall, the galaxy presents as a fairly massive, relatively quiescent system.