The galaxy appears as a relatively compact object. The central region exhibits a bright, concentrated luminosity, suggesting the presence of a prominent galactic nucleus. There is evidence of a disk-like structure, albeit somewhat disturbed or irregular. The color profile shifts from a bluish hue in the inner region to a redder appearance in the outer parts. This could signify ongoing star formation concentrated toward the core, with older stellar populations dominating the outskirts. Faint tidal tails are visible, indicating potential past gravitational interactions or merger events. The object's overall morphology is difficult to classify definitively but might be an elliptical galaxy or an unusual spiral. 
