The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse light distribution with no distinct spiral arm structures. Its overall shape is elongated, with a high degree of ellipticity. The central region displays a higher concentration of luminosity, indicating the presence of a galactic bulge. The color profile suggests an older stellar population, with a reddish-yellow hue dominating the central regions, transitioning to a bluer, but still faint halo. There is no apparent evidence of active star formation regions or significant dust lanes within the visible spectrum. The galaxy appears relatively undisturbed, showing no signs of ongoing major mergers or tidal interactions.
