The galaxy presents as a moderately sized, lenticular or early-type spiral galaxy, exhibiting a generally smooth morphology. It appears elliptical in shape, with a high degree of roundness, showing no significant signs of distortions typically associated with major mergers or tidal interactions. There is a slight color gradient observed, with the central region appearing more yellow or red, suggesting a higher concentration of older stellar populations or dust obscuration. The outer regions are fainter and bluer, possibly indicating the presence of some younger, star-forming regions, though these are not prominently defined. Overall, the galaxy appears to be relatively quiescent in terms of ongoing star formation activity. Faint, extended halo structures may exist, but are difficult to resolve with the available image quality. There are no discernible spiral arms or a prominent central bulge.
