The galaxy presents a generally smooth appearance, with a discernible central bulge that dominates its overall structure. The light from the bulge exhibits a bluish hue, potentially indicating the presence of a younger stellar population. Extending from the central region are faint, diffuse features, possibly indicative of spiral arms or tidal disturbances. These are subtle and don't present a clear, well-defined spiral structure. There is an extension that may be a tidal tail, or a secondary spiral arm. Overall the galaxy is more circular than oblong. Evidence suggests that the galaxy may be undergoing minor gravitational interactions, exhibiting some structural distortion.
