This galaxy exhibits a morphology consistent with an elliptical type, though it shows some features that suggest possible past interaction or disruption. The central region is dominated by a bright, relatively smooth, and featureless bulge. A faint, elongated structure extends outward from one side of the bulge, displaying a color gradient from yellowish to reddish as it extends further outward. This plume-like feature suggests potential tidal debris or a disrupted spiral arm resulting from a past interaction. The galaxy appears moderately flattened. The color indices suggest a galaxy populated by older stars, particularly in the extended structure, with the bulge displaying bluer colors than the tidal feature. Overall, the galaxy presents characteristics of both a mature elliptical system and evidence of a past or ongoing interaction that has influenced its morphology. Further spectroscopic analysis would be required to fully characterize the stellar populations and kinematic signatures within the galaxy and its extended structure.
