The galaxy appears to be a spiral galaxy, likely seen edge-on, as it has a pronounced elongated shape. The central bulge is bright and has a yellowish hue, suggesting an older stellar population. The disk of the galaxy exhibits a bluer coloration at the outer edges, possibly indicating more recent star formation in these regions. It does not show any distinct spiral arm structures, as they are obscured by its orientation and distance. There are no signs of significant mergers or tidal disturbances. It appears relatively isolated, and its overall morphology suggests it is an evolved system with a significant bulge component.
