This galaxy exhibits a roughly lenticular morphology, appearing as a flattened disk viewed at an oblique angle. The overall color is predominantly blue, suggesting the presence of younger, hotter stellar populations. There is a subtle central bulge, which appears slightly more concentrated and less blue than the surrounding disk. Faint, diffuse extensions are visible, particularly on either side of the disk. No distinct spiral arm structure is readily apparent, nor are there signs of a prominent dust lane. The overall structure is mildly disturbed, possibly indicating a past or ongoing interaction, but it is also possible this feature is simply a morphological characteristic of the galaxy itself.
