The galaxy exhibits a notable disc structure, appearing somewhat inclined relative to our line of sight. The central bulge appears prominent, contributing significantly to the overall luminosity of the galaxy. Spiral arm structures are discernible, suggesting ongoing star formation activity within the disc. There are multiple potential merging events present. The inner region of the galaxy displays a high degree of light concentration, possibly indicating an older stellar population within the bulge. The overall color suggests a mix of stellar populations with younger, bluer stars present within the spiral arms and older, redder stars concentrated towards the central bulge. The galaxy appears relatively smooth and moderately concentrated, suggesting a later-type spiral classification. The galaxy has an elliptical shape.
