The galaxy appears to be an elliptical type, with a generally smooth and rounded morphology. There is no apparent spiral structure or bar. The core region exhibits a higher concentration of luminosity, fading gradually towards the outer edges. The color profile appears relatively uniform across the galaxy, with a slightly yellowish-white hue. There are no visually discernible signs of significant star formation or dust lanes, which is consistent with an older stellar population. No indications of ongoing major mergers or tidal disturbances are observed in this image.
