The galaxy presents as a moderately bright, elliptical system with a smooth, featureless morphology. Its color profile suggests a more evolved stellar population, exhibiting a reddish hue, indicative of older, cooler stars dominating the light output. There is no apparent spiral structure or prominent dust lanes. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or mergers in the immediate vicinity, although there is a slight distortion in its overall shape, possibly hinting at a past interaction or minor disturbance. Its round shape, with a slight oblong appearance, is likely due to it not being perfectly aligned to our line of sight. The overall structure appears smooth and concentrated, with a gradual decline in surface brightness from the core to the outer regions.
