The galaxy presents as a generally elliptical morphology, elongated in shape with a high degree of central concentration. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. Color gradients are subtle, with a yellowish hue dominating, indicative of an older stellar population and limited ongoing star formation. There is no clear evidence of tidal features or ongoing mergers, the overall structure appearing settled and undisturbed. The galaxy's estimated size indicates a relatively large physical extent.
