This galaxy presents as an edge-on or nearly edge-on disk galaxy. The central bulge is quite prominent and appears to be relatively large and elliptical in shape, with a smooth, concentrated light profile indicating an older stellar population. The disk itself is elongated and thin, exhibiting a subtle color gradient, transitioning from a yellowish hue in the central regions closer to the bulge, to a slightly bluer color towards the outer edges, suggesting ongoing or recent star formation in these regions. There is no clear indication of spiral arm structure or significant dust lanes visible, but it may be difficult to see such features due to the viewing angle. The overall morphology suggests this is likely an older, relatively undisturbed galaxy that has undergone significant bulge formation. There does not appear to be evidence of a major merger or significant tidal disruption.
