The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology. The light profile suggests a lack of prominent spiral arms or a well-defined disk structure. It exhibits an overall elliptical or spheroidal shape. The color index suggests it may be composed of an older stellar population. There is no evidence of significant ongoing star formation or dust lanes within the galaxy. Based on these morphological characteristics, the object is possibly an elliptical galaxy, potentially an early-type galaxy nearing the red sequence. There are some possible signs of minor tidal disturbances, but they are quite small. No other interacting galaxies are near the host galaxy.
