The observed galaxy presents as a disk galaxy, oriented approximately edge-on relative to our line of sight. The overall structure appears relatively smooth, with a notable central bulge dominating the luminosity profile. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population and lower star formation rate in this region. A fainter disk is visible extending outwards from the bulge. The disk appears slightly bluer in color than the bulge, possibly indicating the presence of younger, hotter stars and ongoing star formation within the disk. There is no clear evidence of strong spiral arm structures or significant dust lanes along the plane of the disk in this image. No obvious signs of interaction or merging are apparent in the immediate vicinity of the galaxy. Overall, the galaxy appears as a moderately luminous, relatively undisturbed disk galaxy with a prominent bulge component.
