The galaxy presents as a somewhat disturbed system, possibly undergoing a merger or interaction. The primary body of the galaxy exhibits a diffuse morphology, lacking a distinct spiral structure. There is an amorphous central concentration with a yellowish hue, suggestive of an older stellar population. Fainter, bluer extensions emanate from the central region, particularly on the left side, which may indicate regions of more recent star formation. An apparent second, smaller object is interacting with or in close proximity to the main galactic body. This secondary object appears as a less concentrated blob of yellowish light. The galaxy displays some irregularity, with a fraction of light coming from regions outside of a smooth profile.
