The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region that appears a yellowish-orange hue. This suggests an older stellar population dominating the core, with potentially diminished star formation. The outer regions of the galaxy show a bluer tint, indicating the presence of some younger, hotter stars and ongoing star formation, though at a seemingly lower rate than the core experienced in the past. There is a subtle indication of a disk component, but no spiral arms. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent major merger events or tidal disruptions. The light distribution is fairly symmetrical, and it exhibits a well-defined edge, further suggesting a relatively relaxed state.
