The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile. A distinct, bright core is present, indicative of a possible active galactic nucleus or a dense stellar population within the bulge. Surrounding the core, a more diffuse halo of light extends outwards, gradually fading into the background. There are hints of a slight elongation, deviating from a perfect circular shape. No distinct spiral arms or dust lanes are discernible within the image, supporting the classification as an elliptical galaxy. The overall color appears yellowish-white, suggesting a predominantly older stellar population. No evidence of ongoing major mergers or significant tidal disturbances is apparent. There may be minor disturbances present but cannot be confirmed with the image.