The galaxy presents as a moderately sized, somewhat diffuse spiral or disk galaxy with a noticeable central bulge. The color indices suggest active star formation, primarily based on the bluer color, especially noticeable on one side of the galaxy. Although the image lacks high resolution, there is an impression of a possibly barred spiral structure, with what appears to be a slight asymmetry to its shape and potentially faint spiral arms or disk features extending from the bulge. There may be minor disturbances, such as asymmetries, present which could indicate a potential minor merger or tidal interactions, but this cannot be confirmed without a higher resolution image. The overall shape suggests it is a disk galaxy viewed at a slight inclination and at a relatively close distance to our own based on the light profile. The magnitude suggests that it is a relatively faint object.
