The galaxy appears as a slightly elongated, lenticular-like object. Its light profile suggests a centrally concentrated bulge surrounded by a fainter, more diffuse disk. The bulge exhibits a yellow-orange hue, indicating an older stellar population and minimal ongoing star formation. The disk, in contrast, shows a slightly bluer color gradient, suggestive of younger stars. The galaxy's structure does not show any signs of major disturbances or tidal features, indicating it's likely not undergoing a major merger. There is very little dust absorption visible, meaning there is likely only a small amount of dust present within the galaxy. The overall appearance implies that this galaxy has a relatively low specific star formation rate.
