The galaxy presents a generally smooth, elliptical morphology, with no readily apparent spiral arm structures. Its shape is more disc-like than circular. The light distribution is centrally concentrated, exhibiting a bright, yellowish-orange core that gradually fades towards the outer regions. This color suggests an older stellar population, potentially dominated by evolved stars. Some low level evidence points to disturbance or interaction with another body. I estimate its mass to be large, and has a low to moderate amount of star formation activity.
