The galaxy presents as an edge-on spiral, exhibiting a pronounced central bulge. The bulge appears relatively smooth and somewhat rounded. A faint, disklike structure extends outwards from the bulge. The color gradients within the galaxy suggest a distribution of stellar populations and dust. The central region displays warmer hues, possibly indicating older stellar populations or dust obscuration, while the outer regions exhibit cooler colors, potentially indicative of ongoing star formation. There is no immediately obvious evidence of major mergers or tidal disturbances. The galaxy's shape is largely undisturbed, suggesting that it is a relatively isolated system.
