The galaxy presents a somewhat elliptical morphology, appearing nearly edge-on. Its central region exhibits a concentrated luminosity profile, suggesting a significant stellar density, and appears relatively smooth. A faint, extended halo surrounds the brighter central region, gradually fading into the background sky. The overall color of the galaxy appears to be redder, potentially indicating an older stellar population. There are no distinct spiral arms or prominent dust lanes visible, suggesting that it may be either an elliptical galaxy or a lenticular galaxy. There may be a faint disk component.
