The galaxy presents as a relatively smooth, centralized light distribution. The core exhibits a yellowish hue, suggesting an older stellar population. The isophotes appear generally elliptical, although there's a slight deviation, hinting at a minor asymmetry or perhaps an interaction. The overall structure lacks prominent spiral arms or a distinct disk component. The light profile decreases smoothly with increasing radius, lacking sharp breaks or features indicative of recent major mergers. Based on the color profile, it appears the galaxy is not currently undergoing a high rate of star formation.
