The galaxy presents a relatively smooth, featureless appearance. Its overall shape approximates a spheroid, showing minimal deviation from circularity. The light profile suggests a centrally concentrated luminosity distribution, indicative of a substantial bulge component. The color is generally blue-white in the center with the edges trending into redder colors. There's a slight suggestion of spiral structure but it could be from tidal disruption or galactic merging, though such features appear minimal. There is no evidence of a strong active galactic nucleus from this image. The low measured redshift indicates that the galaxy is located at a relatively close distance, meaning this is likely a smaller galaxy. The light profile further points toward this conclusion.
