The galaxy presents as a disk galaxy, viewed at a relatively high inclination. Its overall shape is elongated, with the major axis significantly exceeding the minor axis. The central bulge is prominent and appears smooth with a yellowish hue, suggesting a population of older stars. Moving outwards from the bulge, the disk appears relatively smooth with subtle color variations. There is a hint of bluer star formation regions within the disk, mixed with redder regions likely containing dust. There appears to be no significant ongoing major merger activity. There are no obvious tidal tails or shell structures.
