The galaxy presents an elliptical morphology, elongated along a discernible axis. Its light distribution is characterized by a central bulge with a smooth gradient towards its outer regions. The color profile appears to consist of a dominant yellowish-orange hue. There seems to be some distortion or tidal features that suggest the possibility of an interaction or merging event. The central core presents a more concentrated, brighter appearance. No distinct spiral arm structures are readily observed. Based on the observed color and morphology, the galaxy likely has ongoing but potentially declining star formation activity.
