The galaxy presents a smooth, elongated morphology, appearing cigar-shaped from our vantage point. It exhibits a central, brighter core. The overall color profile indicates a mix of stellar populations, with a subtly bluer hue suggesting ongoing, though potentially low-level, star formation. No signs of major disturbances, such as tidal tails or significant asymmetries, are readily apparent, implying it is currently not undergoing a major merger. The galaxy seems to be a relatively isolated system with no apparent interactions influencing its shape or structure at this resolution.
