This galaxy appears to be a spiral galaxy, although the image resolution limits detailed morphological classification. There is evidence of spiral arm structure, though not sharply defined. These arms show hints of star formation activity within them, with bluer regions possibly indicative of younger stellar populations. The galaxy possesses a central bulge, moderately sized relative to the disk. There may be a weak bar feature. There is no strong visual evidence of a significant merger event or major disturbance; however, the indistinctness of features within the galaxy makes it difficult to completely rule out minor interactions. The overall color of the galaxy suggests a mix of stellar populations, without strong dominance of old or young stars.
