The galaxy presents as a lenticular or early-type spiral structure with a bright, concentrated central bulge. The disk is elongated and appears to be viewed at an angle, although no distinct spiral arm features are discernible. The light distribution shows a smooth gradient, with the brightest region concentrated around the central bulge, fading outwards towards the edge of the galaxy. There is a slight color gradient, with the central regions appearing more blue and the outer regions trending towards redder hues. There are no signs of any major recent merger events. The absence of bright, knotty structures suggests a relatively low current star formation rate. Overall, this galaxy appears relatively evolved, with an established morphology.