The galaxy presents an elliptical morphology with a relatively smooth light distribution. The core region appears as a bright, compact nucleus with a moderate concentration of light. The isophotes display an overall elliptical shape, with a suggestion of slight elongation along one axis. The color profile exhibits subtle variations, with a bluer hue concentrated closer to the center, suggesting the presence of some younger stellar populations or regions of ongoing star formation, albeit at a low rate. The outer regions appear redder, indicating a dominance of older, evolved stars. There is no evidence of prominent spiral arms or a well-defined disk structure. Faint, diffuse light extends outwards from the main body of the galaxy, gradually fading into the background sky, suggesting a large stellar halo. There is some hint of minor irregularities or faint tidal features potentially indicative of past interactions, but these are not particularly pronounced. Overall, the galaxy appears as a relatively quiescent elliptical system with signs of limited recent or ongoing star formation.
