The galaxy exhibits a largely smooth morphology, suggesting a possible elliptical or lenticular classification. A faint, extended halo is present, although poorly defined. There is some indication of subtle structural features potentially indicative of a disk-like component or past interaction. A minor disturbance or possible ongoing merger event cannot be ruled out due to subtle distortions in the galaxy's outer regions. The central bulge is relatively prominent but not overly dominant. The color profile shows a general trend toward redder hues. There is a slight variation in color suggestive of ongoing but relatively low levels of star formation activity. The estimated physical size of the galaxy is intermediate. The observed features lean toward a morphology transitioning from a spiral to an elliptical galaxy.
