This galaxy presents as a moderately luminous object, exhibiting a somewhat irregular morphology. The central region displays a high degree of spheroidal symmetry, appearing largely smooth and dominated by older stellar populations, indicated by its yellowish-orange hue. Extending from the central bulge, a faint disk-like structure is discernable, though its arms lack the high-definition spiral pattern, suggestive of an earlier type spiral or potentially a lenticular galaxy. There is a distinct asymmetrical elongation or possible tidal feature on one side of the main galactic body. This secondary concentration of luminosity could be a satellite galaxy or a region of enhanced star formation triggered by an interaction. The overall low levels of blue light suggest a relatively low rate of ongoing star formation.