The galaxy presents a generally smooth appearance, though with some discernible features suggesting possible disturbances or ongoing interactions. The core is bright and centrally concentrated, indicative of a substantial central bulge. Moving outwards, the light distribution appears more diffuse, with hints of asymmetry in the outer regions. There may be tidal tails or distorted arms, which are subtle but present.

The color profile suggests a relatively old stellar population, with a dominant yellowish-red hue implying the presence of evolved stars. Star formation appears to be low. Based on the morphological characteristics, the galaxy may be undergoing a merger event.
