The galaxy appears as a singular, somewhat asymmetrical object, presenting a moderate degree of internal structure. The morphology suggests it may be an elliptical galaxy with possible disturbances.

The light distribution is not uniform, showing a central concentration with diffuse extensions. There are some slightly more luminous regions embedded within the galaxy, but it isn't clear if these are distinct star forming regions or just variations in stellar density.

Color gradients are present, with a slight tendency towards redder hues in the outer regions of the galaxy and bluer hues centrally. This may indicate a presence of older stellar populations in the periphery and younger populations toward the center. No significant dust lanes are clearly visible, suggesting that we are primarily observing the stellar component. The overall smoothness of the light profile suggests a relatively evolved system. The possible features could indicate some past interaction, though the system does not appear to be a merger.
