The galaxy appears to be a relatively smooth, elliptical-type galaxy. It has a concentrated central bulge that dominates its overall appearance. There is a decrease in luminosity when moving towards the outer regions of the galaxy, with a more diffuse halo. The galaxy exhibits a reddish-orange color, suggesting an older stellar population with lower rates of star formation. The shape is generally round, with only a slight deviation. There is no obvious evidence of a prominent disk structure, spiral arms, or active galactic nucleus. The galaxy does not appear to be undergoing any major merging activity or significant tidal disturbances, with no prominent tails or bridges visible.
