The galaxy presents as a single, relatively smooth structure with a centrally concentrated light profile. It appears roughly elliptical in shape, displaying a high degree of roundness with only a slight deviation towards an elongated form. There is no evidence of spiral arm structures or a prominent disk. Faint, diffuse extensions or tidal features are not observed, suggesting it is not currently undergoing a major merger event. Color gradients are subtle across the galaxy, with a slightly redder hue in the central regions, indicative of older stellar populations. Minimal dust lanes are observed, further supporting a relatively quiescent morphology. The overall appearance suggests this galaxy is a massive, relatively evolved system with a suppressed star formation rate.
