The galaxy appears as a relatively small, edge-on spiral system. It exhibits a pronounced central bulge, appearing yellowish in color, which may indicate an older stellar population. A disk component is present, with hints of bluer light extending outwards. The disk is relatively smooth, with no obvious strong spiral arm features discernible at this resolution. Overall, there isn't any prominent evidence of significant disturbances or ongoing major mergers from visual inspection. The estimated redshift indicates that this is a fairly distant galaxy. The blue color of the outer edges may indicate ongoing star formation.
