The galaxy presents as a fairly smooth, elliptical form, with a moderately concentrated core region exhibiting a bluer hue, suggesting the presence of younger stellar populations and potentially ongoing star formation. The outer regions of the galaxy display a more diffuse profile, with a redder color, indicative of older, cooler stars. Overall, the galaxy appears to be relatively undisturbed, without any obvious signs of major mergers or tidal interactions. Its shape indicates a deviation from a perfectly circular morphology, leaning towards an elongated, cigar-like appearance. 
