This galaxy presents as a relatively face-on spiral, with a bright, concentrated central bulge exhibiting a yellowish hue, suggesting a population of older stars. The disk shows evidence of spiral arms, although they appear somewhat disturbed or flocculent, particularly on one side, where there appears to be a disrupted and possibly tidal stream of material, possibly related to a minor merger event. There's some indication of bluer regions within the disk, implying active star formation areas. The disk is not perfectly smooth. The galaxy displays a moderate redshift, and is estimated to be a relatively massive system with ongoing star formation, though at a rate lower than typically seen in vigorously star-forming galaxies.
