The galaxy presents a generally smooth, somewhat elliptical morphology. It exhibits a concentrated central bulge, appearing luminous and gradually fading outward into a less defined halo. There is no clear evidence of spiral arm structures or distinct dust lanes within the galaxy. The galaxy appears slightly elongated, but not significantly cigar-shaped. There is a hint of a possible minor disturbance in the galaxy's morphology, suggesting a potential past interaction or ongoing accretion event. The color profile across the galaxy appears relatively uniform, showing a consistent yellowish-orange hue indicating a population of older stars. The galaxy does not present any signs of active star formation. 
