The galaxy presents as a primarily smooth, elliptical form, elongated in shape with an apparent cigar-like structure. There is evidence of potential interaction or minor disturbance, indicated by asymmetry and faint extensions in its morphology. Color gradients suggest a central concentration of older stellar populations as seen by a redder hue. The bluer tones present in the extended features suggest ongoing, though perhaps limited, star formation within these regions. The overall appearance is consistent with a massive galaxy experiencing or recently having experienced a minor merger or tidal interaction.
