The galaxy appears to be a disk galaxy viewed at a relatively high inclination. The central bulge is prominent, exhibiting a yellowish hue, suggesting a population of older stars. The disk component shows a bluer color profile, indicative of ongoing star formation. Some irregularities in the outer disk suggest possible minor gravitational interaction, though a distinct merger event is not readily apparent. The overall shape is elongated, presenting a moderate deviation from a perfectly circular form. There is a hint of faint spiral arm structure within the disk, but the resolution limits detailed observation. Based on the overall morphology, the galaxy is likely a spiral galaxy with a significant bulge component.
