The galaxy appears to be a disk galaxy, seen at a moderate inclination. There is evidence of a central bulge component which appears slightly yellowish in color. The galaxy's disk is elongated and has a bluish tinge, suggesting the presence of younger stellar populations. The galaxy displays a generally smooth appearance, with minimal indication of strong spiral arm features or prominent dust lanes within the disk. A slight asymmetry may be present in the outer regions, potentially indicating some gravitational disturbance or interaction, however it does not show clear signs of an ongoing major merger event.
