The galaxy exhibits a roughly elliptical morphology, though displaying some features suggestive of a disk component. The central region presents a bright, concentrated luminosity, potentially indicative of a bulge. The outer regions appear more diffuse, with a suggestion of spiral arm structure, though this is not sharply defined. There is a color gradient observed, with the central bulge appearing more yellow/orange in hue, transitioning to a bluer tint in the outer regions. This color difference could imply a difference in stellar populations, with older, redder stars dominating the bulge and younger, bluer stars more prevalent in the arms. The galaxy shows no obvious signs of major interaction or tidal disturbance, although there is a slight asymmetry in the outer disk indicating minor disturbances. The overall appearance suggests a galaxy with a substantial bulge component and a moderately active star formation rate, particularly in its outer regions.
