The galaxy presents as a relatively smooth, elliptical-like structure with a prominent central bulge. The bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars. Extending outwards from the bulge is a fainter, more diffuse halo or disk, though the lack of distinct spiral arm structure points away from a classical spiral galaxy. The color gradient suggests older stellar populations dominate, with a yellowish hue observed in the central regions, indicative of aging stars. The overall shape is elongated, appearing somewhere between round and cigar-shaped. There is no visually discernable evidence of any major merger events or significant tidal disturbances.
