The galaxy appears to be an elliptical type, exhibiting a smooth and relatively featureless morphology. The light distribution suggests a centrally concentrated spheroid, with a gradual decline in surface brightness moving outwards. The overall shape is elongated, resembling a cigar or football-like structure.

There is a slight color gradient apparent, with the core exhibiting a more yellowish-orange hue, potentially indicating an older stellar population. Fainter bluish-white regions are also visible, suggesting the presence of a younger population of stars. There is no evidence of spiral arms or a prominent disk. No signs of recent or ongoing major merger activity are evident. The galaxy seems isolated.
