This galaxy presents a relatively smooth, elliptical morphology, exhibiting a moderate degree of central concentration. The color gradient suggests a higher proportion of older stellar populations. While there is no strong evidence of spiral arms, a slight asymmetry in the distribution of light may indicate a minor interaction or disturbance. The overall red color suggests ongoing, but low level, star formation activity. The galaxy appears to be fairly isolated, without any obvious signs of a major merger event in its recent past, although a potential merger event cannot be ruled out due to the morphology's smooth shape and the slight disturbance of light.
