The galaxy appears to be a luminous, centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy display a subtle color gradient, transitioning to a redder shade as distance from the center increases. No distinct spiral arm structures or significant dust lanes are visible. There appears to be only a very minor indication of disturbance and no obvious evidence of ongoing mergers or tidal interactions, and the shape is mostly round.
