The galaxy presents a smooth, elliptical morphology. Its overall shape appears elongated, tending towards a cigar-like appearance rather than a perfectly round form. The central region exhibits a bright, concentrated luminosity, suggesting a significant density of stars or possibly the presence of an active galactic nucleus. A subtle hint of a disk-like structure or faint, disturbed features can be seen extending from the primary body, implying some interaction or past merger event. The color profile indicates a dominant population of older stars, with a blue shift in the galactic center.
