The galaxy appears as a single, relatively smooth object with an elliptical morphology. It exhibits a central concentration of light, suggesting a prominent galactic nucleus or bulge. The galaxy's color is yellowish-orange, indicative of an older stellar population with lower levels of ongoing star formation. The overall shape leans towards being cigar-shaped rather than perfectly round. There might be evidence of minor disturbances or interactions, potentially hinting at past or ongoing merging activity, but this is not definitively apparent. The system does not show any strong signs of spiral arms or a defined disk structure.
