The galaxy presents as a somewhat elongated, cigar-shaped structure, indicating a possible elliptical morphology, though some disk features cannot be ruled out. The light distribution appears relatively smooth with a central concentration, but with some irregularities suggesting minor disturbances. The galaxy exhibits a color gradient, transitioning from a redder hue in the central region to slightly bluer tones in the outer areas. This may indicate a difference in stellar populations, with older, redder stars dominating the center and younger, bluer stars possibly present in regions of recent star formation in the surrounding areas. There is no strong evidence of a major ongoing merger, although the morphological irregularities could be indicative of past interaction or accretion events. The galaxy shows a moderate degree of star formation. Overall, the galaxy appears to be a transitioning system, possibly evolving from a star-forming spiral to a quiescent elliptical galaxy through processes of interaction and internal evolution.
