The galaxy presents as an elliptical morphology with an overall smooth structure. The central region exhibits a higher concentration of light, appearing almost spherical and with a yellowish-orange hue, indicating an older stellar population. Fainter extensions of diffuse light are observable, stretching outwards from the core. The overall shape is elongated, but not significantly so. There is no distinct dust lane or spiral arm structure visible. A possible companion galaxy is detected close to the primary galaxy. There is a hint of tidal disturbance or interaction between the companion and primary galaxy. 
