The galaxy presents a smooth, largely featureless appearance, suggesting an elliptical morphology or a spiral galaxy viewed at a significant inclination. The dominant color is a yellowish-orange hue, indicative of an older stellar population and relatively low ongoing star formation. There is a slight elongation in its form, falling somewhere between round and cigar-shaped. A small, slightly bluer secondary object is observed in close proximity, which appears to be causing minor disturbances in the main galaxy. This could be a dwarf galaxy undergoing a minor merger or a tidal interaction. The overall structure lacks distinct spiral arms or a prominent central bulge, further supporting the assessment of an elliptical type or a late-type spiral with a heavily obscured structure.
