This galaxy exhibits a generally smooth morphology with a slight degree of ellipticity, appearing somewhat cigar-shaped. It presents a clear central bulge that is bright and concentrated. The surrounding disk is also smooth and lacks defined spiral arms or significant dust lanes. There may be some minor disturbances in the galaxy's outer regions suggesting a prior minor interaction or merger event. The galaxy exhibits a color gradient, with the central bulge appearing redder and the outer disk showing a bluer hue. This color difference is likely due to the presence of older stellar populations in the bulge and ongoing star formation in the disk. 
