The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears fairly uniform across the galaxy, with a slight radial gradient, brighter towards the core. There is no strong evidence of spiral arms or a prominent disk component in this image. The color appears to be slightly reddish, suggesting an older stellar population with less ongoing star formation, and perhaps an absence of younger, bluer stars. The galaxy is generally round in shape. There is no strong evidence of any ongoing major merger events or significant tidal disturbances.
