The galaxy presents as a smooth, elliptical-like structure with a noticeable central bulge. The overall color gradient suggests older stellar populations are dominant. The galaxy's light profile is concentrated toward the center, and the shape is elongated, appearing cigar-shaped. Faint blue hues are visible in the outer regions, possibly indicating recent star formation, although it appears to be at a low rate. There are no clear signs of spiral arms or significant dust lanes. No major distortions or tidal features are apparent, suggesting it is likely not undergoing a major merger. Subtle irregularities might indicate minor disturbances.
