The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its overall color is yellowish-orange, possibly indicative of an older stellar population with fewer young, blue stars, and enhanced dust absorption of blue light. There is a gradual decrease in luminosity from the center to the edges, lacking any distinct spiral arm structures or prominent dust lanes. The galaxy is nearly circular in appearance, suggesting that it is either a true elliptical galaxy, or we are observing a spiral galaxy face-on. The lack of any significant distortions or tidal features suggests that the galaxy is not currently undergoing a major merger. Based on its red color and lack of features, it exhibits very little to no star formation activity. Slight irregularities or disturbances in the outer regions cannot be ruled out at this resolution, but the dominant impression is one of a relaxed, evolved system.
