The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated luminosity profile. The core appears bright and yellowish-white, indicating a likely older stellar population. The outer regions are less defined, transitioning into a faint halo with a reddish tint, which might be caused by a low level of dust extinction or a population of older, redder stars. The galaxy displays a flattened shape, deviating slightly from a perfect circular form. There are no obvious signs of spiral arms or significant dust lanes. The overall texture appears smooth, suggesting a lack of recent major mergers or active star formation within the main body of the galaxy. The galaxy appears to be relatively isolated in the image.
