The galaxy presents as a relatively compact, disk-shaped structure with an apparent bulge. The central region exhibits a concentrated luminosity, indicating a probable high density of stars or an active galactic nucleus. The galaxy's disk shows some asymmetry and irregular features, suggesting possible ongoing interactions or disturbances. There's evidence of possible faint spiral arms or tidal tails extending from the main body, although these features are not sharply defined. Color gradients are observed, with the central bulge appearing more yellow/orange and the outer disk showing hints of bluer hues, indicating varying stellar populations and potential regions of active star formation. The overall structure indicates a system experiencing some level of dynamical evolution, possibly involving minor mergers or gravitational interactions.
