The galaxy presents as a relatively smooth, centrally concentrated structure with a generally elliptical morphology. There is a slight elongation, but overall the shape appears close to round. The central region displays a higher surface brightness, gradually fading towards the outer edges. There are no obvious spiral arm structures or prominent dust lanes visible in this image. No other galactic nuclei in the surrounding area suggest an ongoing or recent major merger event. There is a subtle asymmetry or minor distortion in the galaxy's outer halo, which could indicate a past interaction or minor disturbance. The color appears to be dominated by light in the redder part of the spectrum, with less blue light observed, which may indicate the presence of an older stellar population or a relatively low current star formation rate.
