The galaxy presents as a largely featureless, elliptical-like structure with a smooth light distribution. The core exhibits a concentrated, bright yellowish hue, suggesting an older stellar population. This central region gradually fades into a more diffuse outer halo, exhibiting a slight reddish tint. There is no clear evidence of spiral arms, distinct dust lanes, or active star-forming regions visible in the image. The galaxy appears largely undisturbed, lacking significant tidal features or indications of an ongoing major merger event. The morphology suggests a system dominated by evolved stars with a relatively low ongoing star formation rate. The estimated physical size indicates a galaxy of considerable scale.
