The galaxy appears as a fairly smooth, centrally concentrated object. It exhibits a generally elliptical morphology, approaching circular. The color profile is relatively uniform across the galaxy, trending toward a yellow-white hue, which may be indicative of an older stellar population. There is little evidence of distinct spiral arms or significant dust lanes within the visible structure. I see a small orange disturbance, suggesting a minor tidal interaction or recent minor merger. The overall appearance suggests a relatively evolved system with comparatively low ongoing star formation.
