The galaxy presents a largely smooth morphology with a concentrated central bulge. It appears elliptical in shape, approaching a circular form. There are indications of a slightly disturbed morphology, hinting at a possible minor interaction or past merger event. The primary body exhibits a yellowish hue, consistent with an older stellar population. Based on the observed color, there may be moderate levels of on-going star formation activity. The absolute magnitude indicates it is a luminous galaxy, suggesting a significant mass.
