The galaxy presents a relatively smooth, elliptical morphology with a bright, concentrated central bulge. The color profile suggests an older stellar population, dominated by redder wavelengths, especially towards the core. There is a faint, diffuse halo surrounding the brighter central region, exhibiting a smoother texture than what is seen in typical spiral galaxies. There is no clear indication of distinct spiral arms or significant dust lanes. The galaxy appears largely undisturbed, showing no prominent signs of recent major mergers or tidal interactions.
