The galaxy presents as a singular, moderately bright object with a slightly elongated profile. The light distribution appears concentrated towards the center, suggesting a substantial central bulge or core. There is a subtle color gradient visible, with a more yellowish or reddish hue concentrated in the central region, potentially indicating an older stellar population. No distinct spiral arms or obvious dust lanes are readily apparent in this image. The overall texture suggests a relatively smooth, featureless morphology, possibly consistent with an elliptical galaxy or a lenticular galaxy seen at a significant inclination. There may be slight asymmetry, but it is not significant enough to suggest a major ongoing merger event.
