The galaxy presents an elliptical morphology, appearing relatively smooth and featureless in the available image. There is little indication of spiral arms or prominent dust lanes. The galaxy exhibits a central bulge that is somewhat brighter than the surrounding halo. Overall the galaxy appears to be exhibiting moderate luminosity, with a slightly redshifted spectra suggesting it's at an intermediate distance. The color indices suggest a population of older stars, consistent with an elliptical morphology. There appears to be some evidence of possible interaction with a small neighbor, but further investigation is needed to determine if this is in fact a merger or galactic collision.

