The galaxy presents as a disk galaxy, viewed nearly edge-on from our line of sight. The central bulge is prominent, appearing large and primarily yellowish, suggesting a high concentration of older stars and a relatively low rate of current star formation within this region. The disk itself is fainter and appears bluer, indicating the presence of younger, hotter stars. It is relatively smooth in appearance, with no obvious spiral arm structure visible. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or ongoing major mergers. There is a slight hint of a boxy shape to the bulge. Overall, the galaxy appears to be a well-defined, late-type spiral galaxy, with a moderate redshift.
