The galaxy presents a primarily smooth morphology. It exhibits an elliptical shape, appearing moderately elongated. The central region displays a concentrated, bright core that is yellowish-orange in color, suggesting an older stellar population. Moving outward from the core, the color transitions to a more subtle greenish hue, possibly indicating the presence of younger stars or emission activity, although this is less prominent. There is no clear evidence of distinct spiral arms or a well-defined disk structure. The galaxy appears relatively undisturbed, without significant signs of ongoing mergers or tidal interactions. Overall, the galaxy seems to be a relatively quiescent system with a dominant spheroidal component.
