The galaxy presents as a single, somewhat elongated object. It exhibits a relatively smooth light distribution with no apparent spiral arms or distinct dust lanes. The central region appears brighter and more concentrated, potentially indicative of a galactic bulge. The color is generally yellowish-orange, suggesting an older stellar population with fewer young, massive stars. There is a noticeable asymmetry in the galaxy's light distribution, with a slightly more extended feature protruding from one side, possibly indicating a tidal interaction or the presence of a dwarf galaxy being accreted. Overall, the galaxy's morphology suggests it is an elliptical galaxy or perhaps a lenticular galaxy with a faint, difficult-to-resolve disk component. There may be some signs of ongoing or recent merger activity influencing the morphology.
