The galaxy presents as a centrally concentrated object with a smooth, diffuse light distribution. The core appears bright and slightly elongated, exhibiting a yellowish-white hue. The outer regions of the galaxy display a subtle blue tint, suggesting the presence of a younger stellar population compared to the core. No distinct spiral arm structures or dust lanes are discernible within the galaxy's morphology. There is a hint of a possible tidal tail or minor disturbance emanating from the galaxy which may be suggestive of a past or ongoing minor merger event, though the disturbance is faint. Overall, the galaxy appears to be a relatively quiescent system.