The galaxy presents an overall elliptical morphology with a prominent central bulge. A disk component is evident, displaying a slight inclination relative to our line of sight. The central bulge exhibits a yellowish-white hue, suggesting a population of older, cooler stars. The disk shows patches of bluer light indicative of ongoing star formation. The galaxy's outskirts seem diffuse, with faint spiral arm structures beginning to form in one quadrant. There is some indication of a minor tidal disturbance or interaction with a smaller companion galaxy to one side. The presence of these features suggests possible ongoing or recent merger activity.
