The galaxy presents a largely smooth morphology, with minimal evidence of spiral arms or significant substructure. The overall shape appears generally round, with a slight deviation towards an elliptical form. The galaxy's color profile suggests a redder hue, potentially indicating an older stellar population with a lower rate of ongoing star formation. There is a subtle hint of a possible minor disturbance in the galaxy's structure, with a faint asymmetry present. No clear signs of a major merger or prominent tidal features are visible in the immediate vicinity.
