The galaxy presents as an elliptical or lenticular type system, displaying a smooth, largely featureless morphology. The light is concentrated towards the center with a high degree of symmetry. It shows an approximate size of 8.6 Kpc. The central bulge exhibits a yellowish or white hue, indicative of an older stellar population with reduced ongoing star formation. Moving outward from the center, there is a slight gradient toward a bluer color, though the overall color remains relatively consistent across the galaxy's visible extent, also suggestive of a mature system. There are very minor disturbances along the galaxy that may suggest it is undergoing a minor merger or tidal interaction. Overall the object appears to be a stable, evolved system.
