The galaxy presents as a somewhat elongated, cigar-shaped object. It exhibits a smooth, diffuse light distribution across its body, suggesting an elliptical morphology. There is no evident spiral arm structure or distinct features such as dust lanes. The color gradient indicates a central concentration of older stars, emitting more reddish light, with a subtle shift towards bluer hues at the outer edges, potentially indicating more recent, albeit modest, star formation activity. There appear to be no signs of major disturbances or merging events, with only minor perturbations potentially present. Overall, the galaxy appears to be relatively isolated and quiescent.
