The galaxy presents an elongated, disk-like morphology, viewed nearly edge-on. A prominent central bulge is observed, exhibiting a yellowish hue, possibly indicative of an older stellar population dominating this region. The disk component appears fainter and thinner, fading into the background sky, with hints of a reddish tint, potentially suggesting ongoing or recent star formation activity, although this is not clearly resolved in this image. There is no evidence of major mergers or significant tidal disturbances affecting its overall structure. The bulge appears to be rounded in shape.
