This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth morphology with little to no visible spiral arm structure. The light distribution is concentrated towards the center, with a gradual decrease in intensity as one moves outward. The galaxy exhibits a slightly elongated shape and has a golden hue, which likely indicates an older stellar population with fewer young, blue stars. There is no visible dust lane or significant signs of ongoing star formation. The overall appearance suggests a relatively quiescent system that has undergone significant evolution. The galaxy's estimated size appears to be moderate, neither particularly large nor dwarf-like. There is some evidence of possible minor disturbance, but nothing major. 