This galaxy presents a somewhat elliptical morphology, showing characteristics of a possible disk system. It appears relatively smooth, with a central bulge that graduates gently into a less defined outer disk. The color profile suggests a higher concentration of older stellar populations within the bulge, indicated by the yellowish hue, compared to the bluer colors in the more diffuse outer regions, implying ongoing star formation. There appears to be a slight tilt relative to our line of sight, giving us a partial view of its disk structure.
