The galaxy appears as a somewhat elongated, diffuse object with a noticeable blue hue. This suggests the presence of a younger stellar population and ongoing star formation activity. The central region is brighter, possibly indicating a higher concentration of stars, but there's no clear, well-defined nucleus visible at this resolution. The overall smoothness in the light distribution points toward a possible early-type spiral galaxy, or a late-stage merger remnant that is nearing completion. Faint, asymmetric extensions may be present along the major axis, suggesting tidal interactions or minor disturbances. There is no strong evidence of active galactic nuclei activity based on this image.
