The galaxy presents as an edge-on spiral with a prominent bulge. The bulge exhibits a yellowish hue, potentially indicating an older stellar population and reduced star formation within that region. A relatively faint disk extends from the bulge, appearing somewhat diffuse with a blueish tint, hinting at a younger, more actively star-forming stellar population in the disk. There are no visible spiral arm structures resolved in this image. The galaxy is mostly undisturbed with no apparent signs of a major merger or significant tidal distortions. 
