The galaxy presents as an elongated, cigar-shaped object with a smooth overall appearance. The color profile suggests a concentration of older stellar populations in the central region, exhibiting a yellowish-orange hue. Moving outward from the core, the galaxy displays a faint blueish tinge, potentially indicative of younger stars or ongoing star formation regions, albeit at a relatively low rate. There is no obvious spiral structure, bar, or significant dust lane obscuration visible in this image. The morphology appears largely undisturbed, with no immediate signs of ongoing major merger activity. There might be a slight irregularity in the outer regions, suggesting a possible minor interaction or tidal disturbance, but the overall structure remains primarily elliptical.
