The galaxy presents as a single, concentrated mass with a smooth and somewhat elliptical profile. The central region exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outwards from the center, the color shifts slightly to a redder tone, though this is subtle. No distinct spiral arms or bar structures are discernible. There appear to be no obvious signs of ongoing major mergers or tidal disturbances, with the overall shape appearing relatively undisturbed. The galaxy appears to be relatively isolated in its immediate vicinity.
