The galaxy presents as a system likely undergoing or having recently undergone a merger event. Evidence suggests a possible interaction between a larger, relatively smooth elliptical galaxy and a smaller, more diffuse irregular galaxy or tidal debris.

The primary component exhibits a centrally concentrated light profile with a smooth, diffuse halo extending outwards. The central region displays a yellowish hue, which may indicate an older stellar population. The overall shape of the primary component is moderately elliptical.

A secondary, smaller component appears connected via a faint bridge of light. It shows a bluer color, potentially indicative of ongoing star formation. The morphology of this secondary component is irregular and disrupted, suggesting tidal forces are acting upon it. This irregular component may be a dwarf galaxy being accreted, or the result of a tidal interaction.

There is potential for a third smaller object in the system, it displays similar color and morphology to the secondary component.

There is a notable lack of prominent spiral arm structure or dust lanes within the system.
