The galaxy presents as a relatively smooth, centrally concentrated system. It exhibits a mostly elliptical morphology, appearing nearly round with only a slight deviation from perfect circularity. The luminosity profile appears to increase steadily towards the center, culminating in a bright, concentrated core. There is little evidence of spiral arms or significant disk structures. The galaxy exhibits a color gradient, transitioning from a yellowish core to a bluer, more diffuse outer halo. There appears to be no major merging event or significant tidal disturbance. There may be some minor disturbance in the outer edges of the halo, however it is difficult to say for sure without further data. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
