The galaxy appears to be a relatively smooth, elliptical-like system. Its morphology indicates a generally featureless structure with a centrally concentrated bulge. The galaxy is noticeably elongated with a slight cigar shape, exhibiting a gradual decrease in luminosity from its core to its outer regions. There is little evidence of defined spiral arms or active star formation regions within the visible spectrum, implying a lack of significant ongoing star formation. There is a slight blue tint on one side of the galaxy, potentially suggesting a small amount of star formation. There are no major mergers or disturbances present. The object is most likely a mature galaxy that is transitioning into a more quiescent phase. 
