The galaxy presents as a highly inclined, edge-on spiral or lenticular system. There is a noticeable central bulge that is bright and appears smooth and moderately concentrated. The disk is elongated and exhibits a relatively smooth texture, with no apparent distinct spiral arm structures visible at this resolution. The color gradient suggests a population of older stars. There are no visible signs of recent major merger activity or strong tidal disturbances, though there is some indication of a minor disturbance.
