This galaxy presents as a relatively smooth, centrally concentrated object. The central bulge is prominent and appears almost spherical, transitioning outwards into a more elliptical shape. The color profile indicates a population dominated by older stars, particularly concentrated in the core, with a redder hue. Fainter, bluer light extends outwards, suggesting some ongoing, albeit subdued, star formation activity in the disk or outer regions. There are no obvious spiral arm structures or significant dust lanes visible, and no signs of major merger activity or tidal disturbances. The overall appearance suggests a galaxy with a relatively high degree of symmetry and internal order.
