The galaxy presents an overall irregular morphology, with a centrally concentrated bright region that is somewhat unresolved in this image. Surrounding this central area is a fainter, more diffuse structure. There is some evidence of faint, asymmetric features extending from the core, potentially indicative of tidal disturbances. The color profile of the galaxy reveals that it's generally blue, transitioning to redder hues toward the outer edges. This could imply a difference in stellar populations, with younger, hotter stars being more prevalent in the center and older, cooler stars dominating the periphery. There might be signs of active star formation occurring within the central region, given its blue appearance.
