This galaxy exhibits a somewhat elliptical morphology, potentially indicative of a disk galaxy viewed at an oblique angle or a transition between spiral and lenticular forms. A central bulge is evident, displaying a yellowish hue, suggesting an older stellar population within this region. Moving outward from the core, a bluer color gradient is observed, particularly along the less pronounced extensions of the galaxy, possibly signaling ongoing or recent star formation within a disk-like structure. The overall structure of the galaxy is moderately smooth, although subtle irregularities and faint wisps may indicate minor disturbances. There is no strong evidence of ongoing major mergers or significant tidal interactions, though a subtle asymmetry could hint at minor past interactions. The galaxy has a red shift, meaning it is likely very far away. 
