The galaxy presents as a moderately inclined disk galaxy. Its central bulge exhibits a concentrated, bright, yellowish-orange hue, suggesting a population of older stars. The disk component displays a less intense, more diffuse color, potentially indicating the presence of younger stellar populations and ongoing star formation activity. Faint spiral arm structures may be present, but the image resolution makes definitive confirmation difficult. The overall morphology appears relatively undisturbed, with no immediately obvious signs of recent major merger events. The galaxy exhibits an approximate effective radius of 9.4 kpc.
