This galaxy exhibits a complex morphology with indications of possible tidal disturbances or ongoing interactions. At its core, there appears to be a bright, concentrated region, possibly indicative of an active galactic nucleus or a dense stellar population. Surrounding the core, the galaxy displays less defined structures. There is a dominant blue color, suggesting the presence of significant populations of young, hot stars, likely indicating ongoing star formation activity. There are some indications of possible disturbances in the overall shape and morphology of the galaxy, but these appear minor. This galaxy does not appear smooth, with some indications of internal structure.
