The galaxy presents as a somewhat elliptical, luminous object with a dominant central bulge. It exhibits a relatively smooth morphology, lacking discernible spiral arms or distinct features beyond a general, diffuse halo. The core region shows a high concentration of light, suggesting a significant population of older stars or potentially an active galactic nucleus, although this is not definitively discernible from the image alone. The color profile appears fairly uniform across the galaxy, without strong color gradients indicating regions of particularly active star formation, though there is a slight blueish hue. Overall, the galaxy appears to be a mature system with a relatively evolved stellar population. There are hints of minor disturbances within the system.
