The galaxy presents a somewhat elliptical morphology, appearing elongated with a moderate axis ratio. It exhibits a dominant smooth, centrally concentrated light distribution, with a relatively high degree of symmetry. There is a subtle color gradient visible, transitioning from a more yellowish hue in the central regions to slightly bluer tones towards the outer edges. This may indicate the presence of younger stellar populations in the outer regions, contrasting with older, redder stars in the core. I note no distinct spiral arms or bar structures visible in the image. There is a hint of minor disturbances or features, suggesting the possibility of past interactions or mergers, although the dominant impression is one of relative quiescence.
