The galaxy presents as a somewhat elliptical structure with a relatively smooth light distribution. Its core exhibits a strong concentration of light, indicating a possible bulge component. The color profile suggests a dominant population of older stars, visible in the yellowish hue of the central region. There is a hint of possible disturbance within the central region, which might be interpreted as an ongoing or recent merger event. Faint extensions emanate from the central area, suggesting possible tidal features or interactions. The outskirts appear less defined, potentially due to low-level star formation or interaction with the intergalactic medium. Overall, the galaxy appears to be in a state of ongoing evolution.
