The galaxy presents as an edge-on spiral, with a prominent dust lane bisecting its central region. The bulge is notably elongated and appears quite luminous, displaying a slightly boxy morphology. The disk appears relatively smooth, lacking the clumpy structures indicative of significant star formation. The overall color profile suggests a population of older stars, particularly within the central bulge, while bluer hues are observed in regions extending from the bulge. There is no evidence of major mergers or significant tidal disturbances in the immediate vicinity. The structure of the galaxy is disturbed, possibly an interaction with a nearby galaxy. The system appears to be quite massive.
