The galaxy presents a slightly elongated morphology, appearing nearly face-on with a high degree of rotational symmetry. There is a prominent central bulge region displaying a relatively smooth light distribution. Surrounding the bulge, a fainter disk is visible. The disk exhibits subtle, diffuse structures that might be indicative of spiral arm fragments or irregular dust lanes, which suggests a late-type spiral or possibly an irregular galaxy. The bluer hue of the galaxy is noticeable, particularly within the disk. The color may be attributed to the presence of younger, hotter stars formed during recent star formation activity. There seems to be a faint, diffuse halo or envelope extending beyond the main body of the galaxy, but it's hard to tell.
