The galaxy presents as a relatively smooth, centrally concentrated object with a noticeable red shift. It exhibits an overall elliptical morphology, though not perfectly rounded, appearing slightly elongated. The color gradient suggests an older stellar population dominating the central regions, indicated by a yellowish hue, with a bluer tinge towards the outer edges, hinting at some ongoing star formation. There is evidence of a slight disturbance in the galaxy's symmetry, perhaps due to a minor interaction or internal dynamics. The galaxy does not appear to be undergoing a major merger, but may have experienced a past interaction that left a subtle imprint on its structure.
