The galaxy presents as an elliptical morphology, exhibiting a high degree of central concentration. The light distribution appears smooth, with a gradual decrease in intensity from the core outwards. There is a subtle color gradient, trending towards redder hues in the central region. The galaxy shows no distinct spiral arm structures or prominent dust lanes. No evidence of strong tidal features, major mergers, or significant morphological distortions are seen, although a very minor disturbance cannot be ruled out. The galaxy is oblong in shape, neither being round nor appearing to be a cigar.
