The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated central region that gradually fades outward. The core presents a yellowish-orange hue, indicative of an older stellar population. Surrounding this central bulge is a fainter, more diffuse halo, also with a yellowish tint. The overall shape is somewhat elongated, transitioning from round to cigar-shaped, suggesting a possible interaction or past merger event. There is a subtle hint of a disturbed morphology, but no clear tidal tails or other obvious signs of an ongoing major merger. The lack of distinct blue regions implies minimal recent star formation activity.
