The galaxy appears as a moderately luminous, slightly elongated object. Its color profile suggests a spectral type trending towards the blue end of the spectrum, hinting at relatively recent or ongoing star formation activity, or it is being seen at its early stage. The central region is characterized by a bright core, indicating a concentration of stars and possibly an active galactic nucleus, although the resolution is insufficient to definitively confirm the presence of an AGN based on morphology alone. The overall structure lacks distinct spiral arms or a prominent disk, classifying the galaxy most likely as an elliptical or lenticular type. There is some evidence of a faint, diffuse halo surrounding the central body, suggesting extended stellar populations or interaction. The object exhibits a smooth profile with a fairly high concentration index, however, it shows some disturbance and maybe in the early stages of merging.
