The galaxy exhibits a generally elliptical morphology, appearing largely smooth in texture. There is a slight deviation from perfect circularity. The light profile is centrally concentrated, showing a peak in intensity near the center. While a distinct bulge component is not immediately apparent, the overall luminosity and morphology suggest a substantial spheroidal component. The galaxy presents a yellowish-orange color, indicative of an older stellar population dominating the light output. There is no clear evidence of spiral arms or a distinct disk structure. Subtle distortions or asymmetries may be present in the outer regions, warranting further investigation into possible past interactions or minor mergers. Overall, the galaxy appears to be an evolved system with minimal recent star formation.
