The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decline in surface brightness outwards. There is a subtle indication of a disk structure. The galaxy exhibits a yellowish hue overall, suggesting an older stellar population and potentially lower rates of ongoing star formation. It appears isolated, with no obvious signs of interaction with other galaxies or major disturbances in its structure, though a small irregular object is seen at its side. The galaxy’s shape is largely round, showing minimal elongation. 
