The galaxy presents as a fairly smooth, centrally concentrated object. It appears to be generally elliptical in shape, exhibiting a high degree of roundness. There is a noticeable color gradient, transitioning from a bluer hue at the core to redder tones in the outer regions. No distinct spiral arm structures or significant dust lanes are discernible within the galaxy's morphology. No signs of major mergers, tidal tails or other forms of significant morphological disruption are observed. The galaxy is likely in a relatively quiescent state.