The galaxy presents as a luminous, yellow-orange object. It displays a generally smooth morphology, with hints of internal structure suggesting it may not be entirely featureless. There is a prominent core and some indication of what might be an ongoing merger or a minor disturbance affecting its overall shape. A secondary light source, close to the main source, is indicative of a merging galaxy, minor tidal effects, or the presence of a bright satellite galaxy in proximity. The galaxy appears roughly rounded, with a slight deviation from perfect circularity. It is emitting strongly across the visible spectrum, with relatively brighter emissions in the redder bands. This is consistent with an older stellar population and relatively low star formation rate. 
