The galaxy presents a generally smooth and amorphous morphology. It exhibits an elongated shape, lacking any clear spiral arm structure. The light distribution appears concentrated towards the center, gradually decreasing in intensity outwards. There are no distinct dust lanes visible, and the color is mostly a yellowish hue, with some faint redder areas on the edges. This suggests an older stellar population and a reduced current rate of star formation. There may be some ongoing gravitational disturbance or interaction with a companion galaxy that is not readily visible in the image, based on its irregular shape.
