The galaxy presents a generally smooth, elliptical morphology. The central bulge exhibits a concentrated, bright, yellowish-gold hue, suggesting an older stellar population. This core region transitions gradually outward, exhibiting a more diffuse halo. The color shifts subtly towards a redder tint, indicative of cooler stars, and lower levels of recent star formation. There appears to be a very slight asymmetry, possibly due to a minor gravitational interaction or a recent accretion event that may have caused a minor disturbance. The overall structure lacks any distinct spiral arms or a prominent disk component. The galaxy appears to be in a relatively quiescent state with a low star formation rate.
