The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a smooth, centrally concentrated morphology. The light profile indicates a relatively high degree of symmetry, with a dominant spheroidal component. There's little evidence of distinct spiral arms or prominent dust lanes, suggesting a well-mixed stellar population. The color gradients suggest a central bulge with older, redder stars, transitioning to slightly bluer hues in the outer disk. There may be some low levels of star formation occurring in the outer regions, as suggested by the bluer light. No major signs of recent mergers or tidal disturbances are visible. The disk component appears to be intermediate in thickness. Overall, the galaxy appears to be in a relatively quiescent state.
