The galaxy appears to be a spiral type, characterized by a prominent, moderately sized bulge at its center. It exhibits a well-defined disk structure. There is a strong central bar feature. Tightly wound spiral arms emanate from the bar region. The arms display a complex structure with some patchiness and signs of active star formation regions. There are more than 4 clearly visible spiral arms. The central bulge displays a yellowish hue, suggesting an older stellar population. The spiral arms exhibit a bluer color, indicative of younger stars and ongoing star formation. There is no evidence of major merging activity or significant tidal disturbances. There is a small amount of dust.