The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology. Its overall shape is elliptical, though some subtle deviations from perfect ellipticity are present. The light profile suggests a high degree of bulge dominance. There is very little evidence of a distinct disk component. 

The galaxy exhibits a colour gradient, with the core appearing slightly redder than the outer regions. There is no clear sign of spiral arm structure, bar features, or dust lanes. This is consistent with the galaxy being a relatively quiescent system, with little active star formation currently taking place. There may be some minor disturbance present, but the evidence for a significant ongoing merger is weak.
