The galaxy presents as an asymmetrical structure, with a generally smooth appearance indicative of an elliptical or lenticular morphology. The galaxy exhibits an irregular color distribution. A distinct, intensely colored region of the galaxy is present, displaying a vibrant blue-green hue transitioning into magenta. This intense color suggests a region of active star formation or potentially an active galactic nucleus. The elongated shape and overall irregular morphology suggest a history of gravitational interaction or possible ongoing merger activity. The presence of a fainter, more diffuse halo, which exhibits a redder color profile than the galactic core, indicating an older stellar population or a higher dust content. The overall size is compact, but with notable asymmetry and irregular features that deviate from a perfectly elliptical profile.
