This galaxy presents as a slightly elongated, disk-like structure, viewed at an angle that suggests it is an inclined spiral or lenticular galaxy. It exhibits a central bulge that appears relatively smooth and concentrated, with a yellow-white hue, indicating an older stellar population. Faint blue-ish light is interspersed within its yellow-white hue.

The surrounding disk shows a subtle gradient in color, with the outer regions appearing slightly bluer than the central bulge, suggesting the presence of younger, hotter stars and ongoing star formation in these areas. The overall morphology seems relatively undisturbed, showing no major signs of tidal interactions or mergers, though subtle asymmetries cannot be ruled out at this resolution. The galaxy appears to be relatively compact, with a noticeable falloff in light intensity from the core outwards.
