The galaxy appears as a single, relatively smooth object, with a bright central bulge surrounded by a more diffuse halo. The central bulge exhibits a yellowish hue, suggesting a population of older stars. The surrounding halo has a faint bluish tint, potentially indicating the presence of younger, hotter stars or some ongoing star formation, although at a low rate. The galaxy appears moderately round in shape, displaying no signs of significant tidal disturbances or ongoing mergers. Overall, the galaxy exhibits characteristics of a relatively quiescent system, possibly an elliptical or lenticular galaxy with a small amount of residual star formation. The galaxy is estimated to be a medium-mass system.
