The galaxy presents as an elongated, disk-shaped structure, oriented nearly edge-on relative to our line of sight. A prominent central bulge is observed, appearing somewhat rounded in shape. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population and/or significant dust obscuration. A thin, flattened disk extends outwards from the bulge, displaying a faint, bluish tint along its outer edges, indicative of ongoing star formation. There is no evidence of any major ongoing mergers or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed.
