The galaxy presents as a relatively compact, centrally concentrated object. The overall color profile suggests a mixed stellar population, with a dominant blue/cyan core indicative of recent or ongoing star formation activity. The outer regions exhibit a more diffuse and red-shifted appearance, potentially reflecting an older stellar population and dust absorption. There is a slight elongation present, suggesting a non-spherical morphology. No clear spiral arm structures or prominent disk features are discernible, but this could be due to the viewing angle or the limitations of the image resolution. There is some potential evidence of minor tidal disturbances or interactions, though further analysis would be needed to confirm this. Overall, this galaxy appears to be a somewhat irregular galaxy, experiencing moderate star formation in its central region.
