The galaxy exhibits a generally smooth morphology, with a slight elongation suggestive of a flattened spheroid. The light distribution is centrally concentrated, appearing brightest towards the core. The object displays a subtle color gradient, transitioning from a yellowish-white core to slightly redder outer regions, with a hint of bluer areas on the edges. This may indicate a declining population of younger, bluer stars toward the outskirts. No obvious spiral arms or dust lanes are discernible, reinforcing a classification as a lenticular or early-type spiral galaxy with the smooth component dominating. There is no clear evidence of major ongoing mergers or significant tidal disturbances, although a very minor disturbance cannot be fully ruled out.
