The galaxy presents as a somewhat elliptical structure, exhibiting a smooth, diffuse morphology. A concentrated, bright central bulge is apparent, displaying a yellowish-orange hue that suggests an older stellar population. The outer regions of the galaxy show a fainter, more subtle greenish tint. There is no evidence of prominent spiral arms or distinct dust lanes. Based on the color gradient, we see a relatively low rate of active star formation. The object shows no signs of major disturbances or ongoing merging events. The galaxy appears largely undisturbed.
