The galaxy presents as a disk galaxy observed at a high inclination angle, nearly edge-on to our line of sight. A prominent central bulge is apparent, exhibiting a smooth, concentrated luminosity profile, likely indicative of an older stellar population. A faint disk extends outwards from the bulge, with a suggestion of obscuration.  There is some subtle clumpy structure present within the disk but without clear indications of spiral arms or active star formation regions. There does not appear to be a strong indication of a recent major merger event or strong tidal interactions.
