The galaxy presents a somewhat elliptical morphology, displaying a dominant central bulge. There is evidence of a disk structure, although it is not viewed perfectly edge-on. The light distribution suggests some level of recent or ongoing star formation, particularly in the disk region, as indicated by the subtle blue hue. No significant signs of tidal disturbances or major merger activity are visible, although there may be minor irregularities that could indicate subtle interaction. The galaxy exhibits an overall smooth appearance, but faint disk-like features are noticeable, extending outwards from the bright central bulge.
