The galaxy presents an overall smooth morphology, exhibiting a concentrated central bulge that fades outwards into a less defined disk. The light distribution appears relatively even across the structure, lacking prominent spiral arms or distinct features usually associated with ongoing star formation. It seems the galaxy may be undergoing a period of quiescence, indicated by the smooth profile and lack of distinct star-forming regions. There are no obvious signs of tidal disturbances or interactions, and the overall form appears largely undisturbed. The color profile suggests a greater concentration of older stellar populations, leading to a reddish hue.
