This galaxy appears to be a relatively smooth, elliptical galaxy with a predominantly yellowish hue, suggesting an older stellar population. The galaxy exhibits a high degree of roundness in its overall shape. There is some evidence of a possible minor disturbance or interaction event. The galaxy seems to be part of a small group, with at least three distinct, concentrated regions of luminosity. The primary central region is the brightest, with two slightly less luminous regions positioned above. There are no prominent spiral arms or dust lanes visible. Based on the observed color, this galaxy likely has a low ongoing star formation rate.
