The galaxy presents as a centrally concentrated, smooth structure. The light profile suggests an elliptical morphology, with a bright, yellowish core that gradually fades outwards. There is no evidence of spiral arms or a distinct disk component in the visible wavelengths. The roundness of the galaxy is very notable, and there is no evidence of disturbance or merging. The color profile is largely homogenous, which could indicate an older stellar population dominating the luminosity. The overall appearance suggests a quiescent galaxy with minimal recent star formation activity.
