The galaxy presents a generally smooth morphology, with a predominantly rounded appearance. There are no distinct spiral arms visible; instead, the light is diffusely distributed. The galaxy exhibits a color gradient, appearing more yellow-white towards the center, with the outer regions trending towards a redder hue. This suggests a possible variation in stellar populations, with older, redder stars dominating the periphery and younger, hotter stars concentrated toward the core. There are no distinct features such as dust lanes or prominent star-forming regions immediately apparent. There is some evidence of a possible minor disturbance within the galactic structure, or possibly evidence of a faint tidal tail.
