The galaxy presents as an elongated, spindle-shaped object, characteristic of an edge-on or highly inclined disk galaxy. Its morphology is smooth and centrally concentrated, suggestive of a prominent bulge. The light distribution exhibits a color gradient, transitioning from a bluer hue at the outer edges to a redder tint towards the central region. The overall red color suggests a stellar population dominated by older, evolved stars, with relatively low ongoing star formation. There is no discernible evidence of major disturbances or mergers in the galaxy's structure.
