The galaxy presents with a shape that is neither perfectly elliptical nor fully disk-like; it appears somewhat elongated with a high degree of central concentration. The light distribution suggests a smooth profile in some sections, but appears distorted with some features in other areas. The primary component of the light from the galaxy emanates from what seems to be a bulge, as indicated by its brightness and central concentration. There appear to be some disturbances in the outer regions. It's difficult to determine the precise nature of these disturbances without higher resolution data, but they appear as minor irregularities in the overall structure of the galaxy. The color gradient suggests a distribution of stellar populations, where the central regions appear bright, and there is a transition to dimmer blue hues towards the outer edges. These observations suggests the possibility of an ongoing or recent minor merging event or other gravitational interaction.
