The galaxy presents as a relatively smooth, disk-like structure. Its overall shape is somewhat rounded, but not perfectly spherical. The core region exhibits a concentrated yellow-orange hue, suggesting an older stellar population and lower rates of ongoing star formation in this area. Fainter, diffuse blue regions extend from the central region, indicating the presence of some younger, hotter stars within the galaxy's outer disk. There is a slight visual asymmetry, with subtle disturbances in the distribution of light that imply a possible past or ongoing interaction or merger event. Lacking a highly defined spiral structure, it may be classified as either a lenticular or a disk-dominated spiral galaxy viewed at an angle.
