The galaxy presents as an edge-on disk galaxy with a prominent bulge. The bulge exhibits a concentrated luminosity gradient, appearing significantly brighter than the disk component. The disk is relatively thin and shows a degree of warping, with a hint of possible spiral structure or dust lanes within it. The light distribution within the disk is smooth, suggesting a well-mixed stellar population. The galaxy's overall morphology is elliptical, with the major axis significantly longer than the minor axis. The galaxy exhibits an overall reddish color, suggesting an older stellar population dominates. There is no evidence of major disturbances or ongoing merging activity, though the subtle asymmetries in the disk suggest a possible minor interaction in its past.
