The galaxy presents a generally smooth and rounded appearance, with a slight elongation. It exhibits a concentrated central bulge, appearing yellowish-white in color, suggesting an older stellar population. Surrounding the bulge is a less defined, bluer, and more diffuse disk. The overall structure hints at a possible lenticular galaxy classification, exhibiting a disk but lacking prominent spiral arms. There are subtle indications of minor disturbances in the outer regions of the galaxy, potentially due to past gravitational interactions or minor merging events. Overall, the galaxy's light distribution suggests that the majority of its stars are located within the bulge, and there is some ongoing star formation activity in the outer disk regions, albeit at a low rate.
