The galaxy exhibits a slightly elongated, cigar-shaped morphology. It appears relatively smooth in structure, without prominent spiral arms or well-defined dust lanes visible in the image. A central, concentrated region shows a yellowish-orange hue. Extending outwards from the center, the galaxy displays a bluish color. This color variation suggests a difference in stellar populations, with the central region potentially dominated by older, redder stars, and the outer regions possibly containing younger, bluer stars, indicative of ongoing or recent star formation. There are no obvious signs of major disturbances, such as tidal tails or strongly asymmetric features, although subtle irregularities in the outer regions cannot be entirely ruled out based on this image alone. Overall, the galaxy appears as a relatively isolated system, though there may be some faint signs of recent or minor disturbances.
