The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless profile. The light distribution suggests it is moderately elongated, displaying an intermediate ellipticity. The central region shows a concentration of light, indicative of a galactic nucleus or core. The color gradient appears fairly consistent across the galaxy, suggesting a relatively homogeneous stellar population, with a possible dominance of older, redder stars. There is no visual evidence of spiral arms or significant dust lanes. Subtle disturbances in the outer regions can not be ruled out based on this image alone.
