The galaxy appears to be a spiral galaxy, seen at a significant angle. A central bulge is visible and shows an elliptical profile, with a bright concentration of light. It exhibits a yellow to orange hue, suggesting a population of older stars. The spiral arms are not tightly wound, and display a mottled texture, indicating active star formation regions. Patches of blue light along the spiral arms are suggestive of young, hot stars. The overall color gradient implies a redder bulge and bluer arms, consistent with stellar population variations within the galaxy. There is visual evidence of potential disturbances or tidal features, which could indicate ongoing or past interactions with another galaxy.
