The galaxy presents a centrally concentrated luminosity profile with a smooth overall appearance. The light distribution suggests an elliptical morphology, but with a slight flattening, placing it somewhere between round and in-between. It exhibits no clearly discernible spiral arm structures or a prominent disk component within the observable bands. The central region displays a yellowish hue, potentially indicating an older stellar population, while the outer regions show traces of blue, suggesting some ongoing, albeit low-level, star formation activity. There is some morphological disturbance in the galaxy, likely either a minor disturbance or a full blown merger. This conclusion is based on the asymmetrical light distribution and some clumpy morphology, making a definite conclusion impossible.
