The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decline in surface brightness moving outward from the core. There is a dominant, bright central bulge, which is a golden-yellow hue, indicative of an older stellar population. Fainter, diffuse light extending outwards appears more red-shifted, suggesting evolved stars dominate the outer regions as well. There is no obvious indication of spiral arm structure or significant dust lanes. The galaxy exhibits a high degree of circularity, with only a very subtle deviation from a perfectly round shape. No major merger events or tidal disturbances are readily apparent, although a very slight irregularity in the outer halo might suggest a minor interaction in the past. Overall, the galaxy appears to be a relatively quiescent system, likely undergoing low levels of star formation.
