The galaxy appears as a moderately bright, elliptical or lenticular type. It exhibits a generally smooth morphology, with a dominant central bulge that appears somewhat circular. The color gradient suggests a higher concentration of older stellar populations within the central region, manifesting as a yellowish hue. There is a subtle indication of a flattened disc component surrounding the bulge. No prominent spiral arms or dust lanes are discernible. The overall structure suggests a system that has largely exhausted its gas reservoir and is experiencing relatively low levels of ongoing star formation, or is quiescent. There may be evidence of minor gravitational disturbance or interactions with neighboring galaxies, as indicated by faint asymmetrical features or tidal tails, though they do not indicate an ongoing major merger event.
