This galaxy presents as a disk galaxy viewed at an intermediate angle, possibly leaning towards edge-on. There's a noticeable central bulge that appears relatively bright and concentrated with a yellowish hue. This would suggest an older stellar population within the bulge.

The disk component exhibits a bluer color, indicating ongoing star formation, though it doesn't appear to be heavily dominated by bright, discrete star-forming regions. The disk appears relatively smooth, with some subtle indications of spiral arm structure, but they are not sharply defined.

One side of the galaxy seems slightly more extended or disturbed. I wonder if it is exhibiting minor disturbances, possibly due to a past interaction, or if it is just a result of the galaxy's internal dynamics. There is no obvious signs of strong tidal features or a clear merger, but there is an indication that something is interacting with the galaxy.
