The galaxy presents as a relatively smooth, elliptical structure. Its central region exhibits a concentrated, yellowish-white hue, indicative of an older stellar population. Moving outward, the light gradually fades to a bluish-white fringe, suggesting the presence of some younger, hotter stars, or possibly a scattering effect. The overall shape is elongated, appearing cigar-shaped rather than perfectly spherical. There are no clear signs of spiral arms, bars, or major disturbances, nor is there evidence of a recent or ongoing major merger. The galaxy does not appear to be actively forming a significant amount of new stars, but could be in a region of space with a very tiny amount of active star formation.
