The galaxy appears as a relatively smooth, elliptical-like structure. The light profile suggests a centrally concentrated mass distribution. There is evidence of a slight disturbance in the galaxy's morphology, potentially due to minor gravitational interactions with another galaxy, or internal processes. The color distribution is primarily reddish-yellow, indicating an older stellar population with less active star formation. The central region exhibits a brighter, more condensed core. Overall, the galaxy seems to be an evolved system, potentially in the process of merging with another galaxy.
