The galaxy presents as a centrally concentrated object, exhibiting a high degree of radial symmetry. Its morphology appears largely smooth, with a general lack of resolved features or distinct spiral arm structures. The primary visible characteristic is a centrally bright, roughly circular bulge region. The light profile fades gradually outwards from the center, suggesting a diffuse outer halo or envelope. There is a slight elongation, deviating somewhat from a perfect circle. No significant tidal features, such as streams or tails indicative of recent major merger events, are discernible. There is no clear indication of the presence of dust lanes or strong star-forming regions. The galaxy's dominant color is yellow-orange, suggesting a stellar population dominated by older, redder stars.
