The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core. The light profile appears to decline gradually from the center outwards, suggesting a relatively uniform distribution of stars. The color is predominantly yellow-orange, consistent with an older stellar population. There is no clear evidence of spiral arms or significant dust lanes. The overall appearance suggests an evolved galaxy with minimal ongoing star formation and a high degree of spheroidal symmetry, with some signs of slight ellipticity. There are no indications of tidal tails or other disturbances indicative of a major merger.