The galaxy appears relatively compact and concentrated, exhibiting a dominant red hue in its outer regions. The core presents a brighter, possibly more active region with a distinct magenta-white color gradient, suggesting intense activity or a different stellar population composition compared to the outer areas. While the overall morphology is generally smooth, there is a hint of asymmetry or disturbance indicated by some subtle non-uniformity in the light distribution. There are indications of slight tidal disturbances with hints of minor merging activity. The internal structure shows no discernible spiral arms or distinct disk features.
