The observed galaxy appears as an elongated structure, presenting an edge-on perspective from our line of sight. A distinct central bulge is visible, appearing bright and somewhat rounded. The disk component is narrow and extends outwards from the bulge, with a relatively smooth appearance along its length. The color gradient suggests a higher concentration of older stellar populations in the central bulge, shifting to bluer hues in the disk, possibly indicating ongoing star formation within the disk regions. There are no obvious signs of tidal disturbances or major mergers, although subtle asymmetries within the disk may indicate minor interactions. The galaxy presents a well-defined structure suggesting it is relatively undisturbed.
