The galaxy presents an elliptical morphology. It has a smooth, centrally concentrated bulge exhibiting a yellow-white hue, suggesting an older stellar population. A faint, diffuse disk surrounds the bulge. There appears to be minimal dust extinction obscuring the galactic structure. Overall, the galaxy exhibits a regular, symmetrical form, without any obvious signs of recent mergers or tidal disturbances. There are no readily visible spiral arms or prominent star-forming regions.
