The galaxy presents as an elongated, spindle-shaped structure, consistent with an edge-on or highly inclined disk galaxy. The central region exhibits a brighter, more concentrated luminosity, suggesting a significant stellar bulge. A subtle color gradient is observable, with a slightly bluer hue in the outer disk regions compared to the redder central bulge. This hints at ongoing or recent star formation in the disk. The galaxy exhibits a relatively smooth overall appearance, with no pronounced spiral arm structures or prominent dust lanes immediately apparent in this imaging. There may be some minor tidal features present, suggesting a possible interaction, but more data would be necessary to confirm.
