This galaxy appears to be a relatively smooth, elongated system. The light distribution is not perfectly uniform, with a slightly brighter central region suggesting a concentration of stars and possibly a bulge. Overall, it appears to be a very compact system, with an estimated size of about 4.5 kpc. The galaxy's shape is not circular; instead, it is elongated or cigar-shaped.

The galaxy displays an overall blueish tint, which could indicate a population of hot, young stars, suggesting ongoing, but low, star formation. There is no obvious sign of spiral arms or other significant features like dust lanes. The galaxy does not show any signs of major disturbances or interactions with other galaxies and appears fairly isolated.
