The galaxy presents a largely smooth morphology, suggesting it is likely an elliptical galaxy or a lenticular galaxy viewed at an angle. It appears to have an elliptical shape, exhibiting a slightly elongated form rather than a perfectly circular profile. The light distribution within the galaxy demonstrates a concentrated central bulge region that gradually decreases in intensity outwards. This suggests a higher density of stars is present near the galactic center. Color variations are visible within the galaxy; the central regions exhibit a more yellow-orange hue, indicating a population of older, redder stars. Fainter blue-ish tones are present in the outer regions of the galaxy. These blue tones suggest the presence of younger stars.

Based on its apparent smoothness, it is unlikely that any major merging events are happening in this galaxy. The presence of slight color variations could suggest ongoing, low-level star formation.
