The galaxy presents as a spiral galaxy, exhibiting a moderate bulge. The spiral arms are tightly wound and difficult to distinguish, appearing as a diffuse disk surrounding the central bulge. There is a degree of asymmetry with the presence of one defined arm on the right side. There is a bright central region possibly indicating high stellar density or AGN activity. The galaxy displays a bluish hue, suggesting ongoing star formation, particularly within the spiral arms. No clear evidence of a strong bar feature is observed. There does not appear to be evidence of any major merging events, though this is very difficult to determine with certainty from this image. The galaxy is likely a late-type spiral galaxy undergoing active star formation.
