The galaxy presents as a moderately luminous, compact object with a flattened spheroidal morphology. The overall color gradient suggests a complex stellar population distribution. The central region exhibits a concentration of older, redder stars, while a blue-ish tint toward the outskirts indicates the presence of younger, hotter stars, possibly within regions of active star formation. 

The morphology suggests an ongoing or recent merger event, as evidenced by a disturbed structure. There are what appear to be tidal tails or debris trails extending from the main body. These features exhibit a bluer color, further supporting the presence of young stars formed as a result of the merger.

The galaxy shows a relatively smooth light profile with a slight asymmetry, which also supports the possibility of recent or ongoing interactions or mergers.
