The observed galaxy presents as a spiral galaxy with a substantial bulge. The bulge appears as a large, prominent, yellowish-white central concentration of light. The spiral arms are somewhat tightly wound. The disk component of the galaxy exhibits a mix of blue and yellow colors. The arms have mottled textures suggesting the presence of active star formation regions, intermixed with older stellar populations. Some segments of the spiral arms appear less defined, potentially indicating dust obscuration or a lower density of luminous material. There are hints of a bar-like structure extending through the center of the galaxy, and the bulge appears moderately sized in proportion to the whole galaxy. The disk of the spiral galaxy is oriented at a moderate inclination angle relative to our line of sight. There are no obvious signs of a major ongoing merger, but some irregularities could suggest minor disturbances.
