The galaxy appears as an interacting system, exhibiting signs of tidal disruption. The primary galactic body shows a roughly elliptical morphology with a diffuse, extended halo component. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. A secondary, smaller object is visible nearby, seemingly connected via a faint bridge of material. This secondary object displays a more compact, reddish appearance, suggestive of ongoing star formation or a different stellar population. There is a distorted morphology and uneven distribution of light within the system. These features suggest a galaxy undergoing a merger or tidal interaction.
