The galaxy presents as a spiral galaxy with a prominent, luminous central bulge. The spiral arms, although somewhat tightly wound, are clearly discernible, displaying a two-armed structure emanating from the core. A subtle bar feature appears to traverse the central region. The galaxy exhibits a moderately inclined disk. The blue-shifted light along the spiral arms suggests ongoing star formation, while the bulge appears more yellow-red shifted, indicating an older stellar population. There is no indication of any major merger activity, with the galaxy exhibiting a relatively undisturbed morphology.
