This galaxy exhibits a generally elongated, cigar-shaped morphology. It appears primarily smooth in texture, with a bright, concentrated central bulge or core. The color gradient suggests a higher concentration of older stars towards the center, transitioning to slightly bluer, younger populations in the outer regions, although this distinction is subtle. The galaxy shows no obvious signs of significant ongoing mergers or major disturbances in its structure. There are no clearly defined spiral arms or distinct features like dust lanes visible, suggesting a relatively evolved system. The overall impression is that of a lenticular or early-type spiral galaxy, viewed at an oblique angle.