The galaxy presents a somewhat elongated, cigar-shaped morphology. Its central region exhibits a smoother, more concentrated light distribution compared to its outer edges. Evidence of a disk-like structure is present, though the overall appearance is not that of a well-defined spiral galaxy. There are only subtle, minor disturbances observed in the morphology. The color profile suggests a mix of stellar populations; the central bulge displays a yellowish hue indicative of older, redder stars, while the fainter outskirts show bluer tones, hinting at younger, star-forming regions. Based on the observed characteristics, it's likely a relatively massive system with moderate star formation activity.
