The galaxy presents as a relatively well-defined spiral structure, exhibiting a moderately inclined disk. The central bulge appears to be of moderate size, contributing significantly to the overall luminosity of the galaxy. Faint, but visible spiral arms extend outward from the central region, displaying a somewhat patchy distribution of luminous regions, indicative of on-going star formation within the arms. There is no visual evidence suggesting a recent major merger event; however, minor disturbances in the disk's symmetry cannot be entirely ruled out. A weak bar structure may be present in the central region. The color gradient suggests a higher concentration of older stars within the bulge, while the bluer hues along the spiral arms support the presence of younger stellar populations associated with active star formation. The galaxy exhibits an overall elliptical shape.
