The galaxy presents a distinct, elongated morphology, suggestive of a spiral galaxy viewed at a significant inclination. The central bulge exhibits a bright, concentrated luminosity, indicating a high stellar density. The disk appears relatively smooth and featureless, with a subtle blue hue along its extent, possibly indicative of ongoing star formation. The overall color suggests a mix of stellar populations, with the bulge potentially dominated by older, redder stars and the disk containing younger, bluer stars. No prominent spiral arms or dust lanes are clearly discernible within the visible range, likely due to the high inclination and limited resolution. The galaxy appears relatively isolated, showing no signs of major interaction with neighboring galaxies.
