The galaxy presents as a relatively small, elliptical object with a concentrated, bright central bulge. The bulge exhibits a strong blue-white color, indicating a population of hot, young stars or a possible active galactic nucleus. Surrounding the central bulge is a less defined disk or halo structure, showing a greenish hue. This color suggests the presence of star formation regions containing ionized gas, specifically oxygen emissions, but could also be contamination of the green filter. There may be some evidence of tidal features or minor disturbances in the outer regions of the galaxy, indicating a possible interaction with another galaxy. Overall, the galaxy's morphology suggests it may be undergoing some level of dynamical interaction or recent starburst activity. 
