The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution appears largely homogenous, lacking any distinct spiral arms or bar structures. There's a subtle color gradient observed, transitioning from a warmer, yellower hue towards the galaxy's core to slightly cooler, redder tones in the outer regions. This could indicate a higher concentration of older stellar populations in the central region, possibly accompanied by a relative lack of on-going star formation. Overall, the object appears to be a relatively undisturbed system, exhibiting no obvious signs of tidal interactions or major mergers, although there might be a very subtle asymmetry that suggests a minor disturbance. 
