The galaxy presents as a spiral type, exhibiting discernible spiral arm structures emanating from a central bulge. The spiral arms appear somewhat patchy, indicating regions of varying stellar density and potentially active star formation. The bulge appears of moderate size, contributing significantly to the overall luminosity of the galaxy. There is a hint of a central bar structure bisecting the bulge region. The disk of the galaxy is not perfectly face-on, showing a slight tilt. This tilt obscures a full view of the spiral structure but does not appear to be quite edge-on. There is some disturbance that may be indicative of a minor interaction, the arm shapes do not follow standard patterns. The color suggests a mix of stellar populations, with the bulge exhibiting a yellowish hue consistent with older stars, while the arms appear bluer, indicating the presence of younger, hotter stars. The galaxy appears to be of intermediate size, occupying a noticeable but not dominant portion of the field of view.
