The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and centrally concentrated morphology. The light distribution indicates a relatively high degree of central concentration, suggesting an older stellar population dominating the core. The galaxy shows a gradual decrease in surface brightness from the core outwards with minimal discernible spiral arm structure or significant dust lanes. There appears to be some minor disturbance or tidal features present that suggest a gravitational interaction or possible past merger events. The shape is mostly round. The galaxy exhibits a red color. The size appears to be in line with other galaxies in the local universe.
