This galaxy presents as a spiral galaxy, observed at a redshift of approximately 0.1488, indicating a substantial distance. The galaxy exhibits well-defined spiral arms, predominantly two in number, which tightly wind around a central bulge. The bulge appears moderately sized. There is evidence of a bar structure bisecting the bulge. No significant signs of major mergers or substantial tidal disturbances are apparent in the immediate vicinity of the galaxy, and it appears relatively isolated. The overall morphology suggests ongoing star formation.
