The galaxy presents with a relatively compact morphology. The central region exhibits a diffuse, moderately luminous glow. There is a suggestion of faint, somewhat irregular arm structures extending outward, but these features are indistinct and blend into the background noise. The overall appearance indicates a possible interaction or disturbance in the recent past, disrupting any pre-existing spiral or elliptical symmetry. Evidence points towards a potential ongoing merger event, with possible tidal features hinted at in the outer regions. However, these features are poorly defined.
