The galaxy presents a generally smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. Its overall appearance suggests it is relatively undisturbed, without evidence of ongoing major mergers or significant tidal distortions. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions, indicating a high degree of central concentration. The galaxy exhibits a moderate redshift, suggesting it is at a considerable distance from our own. The estimated size appears relatively compact, with a relatively small effective radius. Based on its color indices, the galaxy is likely composed of an older stellar population, as the redder colors are indicative of a more evolved stellar population. The blue-ish color of the center suggest younger stars and possible recent star formation, although the overall rate of star formation is likely moderate. The galaxy appears to be relatively massive, based on luminosity. 
