The galaxy appears to be a relatively small, faint object. It is slightly elongated, possibly indicating a disk-like structure or tidal distortion. There is a faint, diffuse glow surrounding the central region, suggesting a relatively low surface brightness. The galaxy exhibits a subtle blue hue in its core. The edges of the galaxy appear indistinct and poorly defined, fading into the background sky, indicative of a dispersed stellar population. Subtle signs of morphological disturbance, like slight asymmetry, may point to possible past interactions. Further investigation is required to assess any potential merger activity.
