The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color gradient suggests an older stellar population, with a yellowish-red hue. There is minimal evidence of spiral arms or significant dust lanes. The galaxy's morphology leans toward an elliptical shape, and it shows little sign of recent or ongoing major merging activity. Minor disturbances are possible, but the overall structure appears relatively undisturbed. Overall, the galaxy presents itself as a mature, quiescent system.
