The galaxy presents a generally smooth appearance, with a high degree of central concentration. The light distribution appears relatively even across its structure, with only subtle variations in color. A slight elongation is observed, deviating marginally from a perfect circular shape. There is no obvious spiral arm structure, nor any distinct central bar. The galaxy is dominated by yellowish and reddish hues, suggesting an older stellar population and a low rate of ongoing star formation. There is little evidence of any major disturbances, such as tidal tails or irregular morphology, that would indicate a recent or ongoing merger event. Minor asymmetry is observed, but nothing substantial.
