The galaxy presents a largely smooth and symmetrical appearance. It appears to be a single, well-defined object without obvious signs of spiral arms or a prominent disk structure. The light distribution suggests a concentrated central region, possibly a bulge, which gradually fades into the outer regions of the galaxy. 

Color gradients are subtle, with the central region appearing somewhat whiter compared to the slightly bluer hue of the outer regions. This could indicate the presence of an older stellar population in the core and younger stars in the outer parts of the galaxy, or differential dust absorption. There are no distinct knots or regions of intense star formation visible, implying a relatively low current star formation rate. The overall morphology is consistent with an elliptical galaxy or a lenticular galaxy viewed at a high inclination. There are no clear signs of ongoing major mergers or significant tidal disturbances. Faint, asymmetric features could indicate minor interactions.