The galaxy presents as a diffuse, slightly elongated structure. The central region exhibits a bluer hue, suggestive of ongoing or recent star formation activity and a younger stellar population. Surrounding the central region, the galaxy displays a yellowish-redder color, potentially indicating an older stellar population. There appear to be some minor disturbances in the morphology, possibly suggesting gravitational interactions. The galaxy is neither perfectly smooth nor does it present as a clear spiral or elliptical shape. It has a small angular size, indicating that it is either intrinsically small or distant. Overall, the galaxy is complex and is potentially undergoing some form of dynamical event, such as a minor merger, although without further data, this cannot be confirmed.
