The galaxy presents as a smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with a slight elongation. The light distribution is fairly even, suggesting a lack of significant spiral arm structures. The color gradient transitions from a bluer hue in the central region to a redder, more yellowish tone towards the outer edges. This color gradient indicates a possible variation in stellar populations, with potentially younger, hotter stars dominating the core and older, cooler stars being more prevalent in the outer regions. There is a faint indication of a possible tidal tail or disturbance, though this feature is subtle and requires further investigation to determine its true nature. There are no apparent signs of a major ongoing merger. 
