The galaxy presents as an elongated, disk-shaped system viewed nearly edge-on. The central region exhibits a significantly higher luminosity, appearing as a bright bulge. This bulge appears mostly rounded, with a smoother texture compared to the outer regions. The disk is relatively thin, showing a slight warp, with an apparent truncation in radial extent and no apparent spiral arm structure. The integrated color is a yellow-orange, possibly indicating an older stellar population in the bulge and disk. The overall impression is of a relatively quiescent system, with no evidence of ongoing major merger activity. There are hints of minor disturbances within the disk, but the majority of the galaxy appears relatively undisturbed.
