The galaxy presents as a relatively smooth elliptical or lenticular morphology. Its central region exhibits a bright, concentrated bulge, fading into a more diffuse halo. The galaxy appears slightly elongated, deviating marginally from a perfect circular shape. The color profile suggests a population of older stars, particularly within the central bulge, which appears more yellow. The outer regions show hints of bluer hues, possibly indicating the presence of younger stellar populations, although these are not distinctly resolved into spiral arms or star-forming regions. There is a subtle asymmetry that could indicate some interaction with another galaxy, although there are no clear signs of tidal tails or merging features. Overall, the galaxy presents a well-defined structure with evidence of both older and some younger stellar components.
