The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an overall elliptical morphology, appearing somewhat rounded rather than elongated. There is a slight color gradient observed, with the central region appearing more yellowish, possibly indicating an older stellar population, and the outer regions exhibiting a bluer hue, suggesting the presence of younger, hotter stars. There is no apparent spiral structure or significant dust lanes visible in this image. No obvious signs of tidal disturbances or interactions with other galaxies are immediately apparent. The galaxy appears to be a relatively isolated system.
