The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, exhibiting a slight elongation. The core region is bright and luminous, suggesting a high density of stars. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. There is a subtle color gradient from the core to the outer regions, with the core appearing more yellow-white and the outer regions appearing more blue. This color shift might indicate differences in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars more dispersed in the outskirts. There is no evidence of distinct spiral arms or significant dust lanes. The overall structure suggests a galaxy with a moderately high mass and a moderate rate of star formation. There might be evidence of a very minor disturbance or ongoing interaction, but it is subtle.
