The galaxy presents as an elliptical morphology, seemingly with a largely smooth light distribution. However, there is evidence of disturbance, specifically a possible merger event, which is suggested by the somewhat distorted shape and the potential for a second, smaller galactic core located distally from the main galactic body. The primary body exhibits a concentration of light toward the core, decreasing in intensity toward its periphery. The overall color of the system tends toward the red end of the spectrum, suggesting an older stellar population with relatively low rates of star formation, although there is a patch of bluer light at the lower left side of the galaxy, potentially indicating a small pocket of more active star formation. Given the overall luminosity of the system, it appears to be a relatively large and massive galaxy.
