The galaxy presents as a disk galaxy with a significant bulge component. The morphology appears to be an elongated ellipsoid. The bulge is a yellow-white color, suggesting an older stellar population. The disk shows hints of blue hues, possibly indicative of younger stars and ongoing star formation, albeit at a low rate. The galaxy does not appear to be significantly disturbed or undergoing a major merger event. There may be a slight asymmetry to the disk, potentially hinting at a minor interaction, but no prominent tidal features are visible. The overall appearance suggests an intermediate-mass galaxy with a relatively smooth structure.
