The galaxy presents a largely smooth, elliptical morphology. It appears well-rounded, exhibiting minimal apparent disturbance or features indicative of ongoing mergers. There is a central concentration of light, with a relatively even luminosity gradient extending outwards. There is no apparent spiral structure or distinct disk component visible. The galaxy is relatively compact, with a diffuse halo extending slightly beyond the main body. The color is generally consistent with an older stellar population, appearing reddish overall. This object is likely a mature galaxy with limited ongoing star formation.
