The galaxy presents a moderately smooth morphology, exhibiting a generally elliptical shape. The color profile appears slightly bluer toward the central region, possibly indicative of a population of younger, hotter stars. It appears to have a high degree of central concentration with no significant disturbance and a relatively high probability that it is smooth. There is a suggestion of a faint, diffuse halo surrounding the main body of the galaxy, but the signal is weak. The overall structure lacks any prominent spiral arms or other distinct features and the light distribution transitions smoothly from the core to the outer regions.
