The galaxy presents as an elliptical or lenticular system, exhibiting a largely smooth, spheroidal morphology. The light distribution suggests a centrally concentrated brightness profile. There is little to no evidence of spiral arm structures, suggesting a lack of significant ongoing star formation within a disk component. The color of the galaxy appears generally redder, indicating an older stellar population dominated by evolved stars. The galaxy appears relatively isolated with a slight hint of a minor disturbance or interaction with a small companion galaxy nearby, it is difficult to say for sure due to the image quality.
