The galaxy presents as a flattened elliptical or lenticular form. It appears to be relatively smooth in structure with a high degree of central concentration, evident by the brighter, yellowish core. The luminosity seems to decrease steadily moving outward from the center. The outer regions fade into a fainter, bluer hue, possibly indicating a subtle population of younger stars or a lack of dust extinction compared to the central bulge. There is a very slight hint of a disk-like feature, though no distinct spiral arms are visible. The galaxy's overall shape is elongated, suggesting a possible cigar-shaped morphology, and exhibits no significant signs of interaction or major disturbances.
