The observed galaxy presents an elongated morphology, strongly suggesting a disk-like structure viewed at a relatively high inclination. A prominent central bulge is visible, exhibiting a smooth, concentrated distribution of light. The disk appears significantly fainter and exhibits a bluer hue in comparison to the bulge, indicative of ongoing or recent star formation. The relatively smooth appearance of the disk may suggest either a lack of prominent spiral arm structure or obscuration due to the viewing angle and dust content within the galaxy. The galaxy's overall color suggests a mixed stellar population, with older, redder stars dominating the bulge and younger, bluer stars present within the disk. There is no obvious evidence of significant tidal disturbances or interactions with neighboring galaxies, suggesting a relatively isolated evolutionary history. The structure overall leans towards a later type spiral, tending toward the "edge on" classification.
