The galaxy presents a somewhat irregular morphology, suggesting possible interactions or recent disturbances in its structure. There's a diffuse, nebulous appearance to its light distribution, predominantly bluish in color, indicating the presence of younger, hotter stars and ongoing star formation, though at a modest rate. While a disk-like structure can be inferred, the overall shape appears rather amorphous, with no prominent central bulge. Faint hints of spiral arm structure can be observed, though they lack clear definition. There are no obvious signs of a strong bar feature bisecting the galaxy's center. Overall, the galaxy appears to be a relatively small, low-mass system, with low star formation activity and signs of possible tidal disturbance.
