The galaxy appears as a relatively smooth and centrally concentrated object. Its shape is moderately elliptical, leaning towards an elongated, cigar-like form. The central region exhibits a bright, intense luminosity, likely indicating a dense concentration of stars or an active galactic nucleus. The light gradually diffuses outward from the core. Faint traces of bluer hues are present within the central region, suggesting ongoing star formation, though at a modest rate. The overall structure lacks any prominent spiral arms or significant dust lanes. There are no visually apparent signs of any major ongoing merger events or tidal disturbances.
