The galaxy presents as a relatively smooth, elliptical-like object, exhibiting a central bulge that is bright and concentrated. There's a noticeable color gradient, shifting from bluer tones at its core to redder hues towards the outer edges, indicative of varying stellar populations and potentially, dust distribution. While a disk structure is not immediately apparent, the overall morphology leans towards an early-type galaxy classification. The galaxy appears largely undisturbed with no obvious signs of ongoing major merger activity. It shows a moderate degree of roundness. 
