The galaxy appears to be an elliptical or lenticular type, showing a predominantly smooth, centrally concentrated light distribution. There is a subtle blue tinge in the central region of the galaxy, indicating possible ongoing, but limited, star formation. The object is largely symmetric, but with a slight elongation along one axis, indicating an intermediate roundness. There is evidence of minor tidal disturbances, likely resulting from a past or ongoing interaction with a smaller companion galaxy. This is primarily visible as subtle asymmetry. There are no prominent spiral arms or a well-defined disk, suggesting a relatively old stellar population. The overall color is trending toward redder wavelengths indicating a significant population of older stars, though that subtle bluer region in the center suggests there is still some star formation.
