The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a bright, yellowish-white hue, potentially indicative of an older stellar population. Moving outwards from the core, the color gradually shifts to a more reddish tint, which could be due to the presence of dust obscuration and/or a change in the stellar population. 

The galaxy appears generally smooth in texture, without prominent spiral arms or distinct features. A slight elongation is discernible, suggesting it is not perfectly spherical but rather somewhat oblate. There is a very subtle, faint bluish glow primarily located around the edges of the galaxy, potentially signifying small pockets of ongoing star formation. There is no evidence of a strong dust lane.

The overall structure suggests a relatively evolved system, possibly undergoing a transition towards a quiescent state with reduced star formation activity.
