The galaxy presents as a relatively smooth, elliptical structure. Its overall color appears yellowish-white, suggesting an older stellar population with fewer young, hot, blue stars. The galaxy's shape is closer to an intermediate elliptical, displaying a slight deviation from a perfectly spherical form but showing no evidence of a developed disk structure. There is no immediately apparent spiral arm structure or prominent dust lanes visible. Indications of ongoing or recent major merger events are not evident. The color gradient within the galaxy appears minimal, with the core region exhibiting a similar color profile to the outer regions. There appears to be slight disturbances or asymmetry present, though the overall appearance is that of a fairly relaxed system.