The object presents as a relatively small, lenticular galaxy. Its overall shape is elongated, appearing cigar-shaped. The color profile suggests a dominant population of older stars with some regions of ongoing star formation, apparent as slight bluish tint. The smooth light distribution and lack of spiral arm structures indicate it is a relatively evolved system. There is no prominent central bulge or active galactic nucleus visible, suggesting that any supermassive black hole at its core is not actively accreting material. The galaxy appears isolated, with no signs of major mergers or significant tidal disturbances. The overall structure is well-defined and suggests it is a stable system.
