The galaxy appears to be a relatively smooth, elliptical or lenticular system. There is a high degree of central concentration with no distinct spiral arms or bar structure visible. It exhibits a roughly round morphology, showing only slight deviations from a perfect circle. The color index suggests a galaxy dominated by an older stellar population, with a moderate redshift. The overall structure displays no obvious signs of a major ongoing merger. However, there's a minor perturbation or tidal feature evident, potentially indicating a past or ongoing interaction with a smaller companion galaxy, or some form of internal disturbance. Star formation rate is quite low within this system. The estimated size of the galaxy suggests it is a relatively compact structure.
