The galaxy presents a largely smooth morphology, with a dominant, centrally concentrated bulge. The overall shape appears close to circular, exhibiting only a minor deviation towards a more elongated form. There is little to no evidence of distinct spiral arms or a well-defined disk structure. The galaxy's light profile suggests a centrally concentrated stellar population, potentially indicative of an older stellar population. The color appears to be slightly more yellow and red suggesting that it is composed of older stars. There are no visible signs of tidal disturbances or major merger events.
