The galaxy presents a predominantly smooth morphology. The central region exhibits a concentrated, bright core, transitioning outwards to a more diffuse halo. The overall shape appears somewhat elongated, but with a slight deviation from a perfect ellipse. There is evidence of a possible interaction or minor disturbance in the upper region of the galaxy, with some asymmetry and a hint of disrupted structure. The color profile indicates a likely mix of stellar populations, with the core showing a tendency towards older, redder stars, while the outer regions show a bluer light, indicative of younger stars or ongoing star formation, but at low levels. 
